[{"messageType":"CME","messageID":"20240513-AL-012","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30827/1","messageIssueTime":"2024-05-13T19:09Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Mars, OSIRIS-APEX, Parker Solar Probe, STEREO A)\n##\n## Message Issue Date: 2024-05-13T19:09:08Z\n## Message ID: 20240513-AL-012\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nO-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-13T09:12Z.\n\nEstimated speed: ~1456 km/s.\n\nEstimated opening half-angle: 49 deg.\n\nDirection (lon./lat.): 72/-36 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-13T09:12:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that the CME may impact Mars, OSIRIS-APEX, Parker Solar Probe, and STEREO A (glancing blow).  The leading edge of the CME will reach Mars at 2024-05-16T18:09Z, OSIRIS-APEX at 2024-05-16T03:29Z, Parker Solar Probe at 2024-05-14T19:15Z, and the flank of the CME may reach STEREO A at 2025-05-16T04:00Z (plus minus 7 hours).\n\nLinks to the movies of the modeled event (includes CME: 2024-05-13T09:12:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_ENLIL_CONE_STA_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_ENLIL_CONE_Mars_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240513_115300_2.0_ENLIL_CONE_Osiris_timeline.gif\n\n\n## Notes: \n\nThe source signatures of this CME event (2024-05-13T09:12:00-CME-001) are associated with multiple M-class flares from Active Region 13664 (S17W77), including an M1.2 flare with ID 2024-05-13T08:06:00-FLR-001 which peaked at 2024-05-13T08:20Z, an M1.4 flare with ID 2024-05-13T08:23:00-FLR-001 which peaked at 2024-05-13T08:29Z, an M4.9 flare with ID 2024-05-13T08:47:00-FLR-001 which peaked at 2024-05-13T09:33Z, and an M6.6 flare with ID 2024-05-13T09:36:00-FLR-001 which peaked at 2024-05-13T09:44Z (see notifications 20240513-AL-003, 20240513-AL-004). \n\nThis CME event (2024-05-13T09:12:00-CME-001) and associated flaring activity listed above are also associated with an SEP at STEREO A with ID 2024-05-13T12:44:00-SEP-001 (see notifications 20240513-AL-006, 20240513-AL-007), a modeled SEP Prediction from REleASE: SOHO/EPHIN 15.8-39.8 MeV with ID 2024-05-13T13:10:00-SEP-001 (see notification 20240513-AL-005), an SEP at GOES-P with ID 2024-05-13T14:00:00-SEP-001 (see notifications 20240513-AL-008, 20240513-AL-009), a modeled SEP Prediction from REleASE: ACE/EPAM 15.8-39.8 MeV with ID 2024-05-13T16:19:00-SEP-001 (see notification 20240513-AL-010), and an SEP at SOHO with ID 2024-05-13T18:07:00-SEP-002 (see notification 20240513-AL-011).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"SEP","messageID":"20240513-AL-011","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30826/1","messageIssueTime":"2024-05-13T18:39Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP (SOHO)\n##\n## Message Issue Date: 2024-05-13T18:39:22Z\n## Message ID: 20240513-AL-011\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by SOHO.  The flux of one or more of the >15.8 MeV protons channels exceeds 10^(-1) pfu/MeV starting at 2024-05-13T18:07Z.\n\nNASA spacecraft at the L1 and near-Earth orbits can be impacted.\n\nActivity ID: 2024-05-13T18:07:00-SEP-002.\n\n## Notes: \nData gap in SOHO from 2024-05-13T14:27Z - 2024-05-13T18:07Z, with the threshold crossed once data returned at T18:07Z, so the true start time is unknown.\n\nEarlier solar energetic particle event prediction by MODEL: REleASE:SOHO/EPHIN 15.8-39.8 MeV with a 2024-05-13T13:10Z event time (see notification 20240513-AL-005), and by MODEL: REleASE:ACE/EPAM 15.8-39.8 MeV with a 2024-05-13T16:19Z event time (see notification 20240513-AL-010).\n\nEarlier solar energetic particle event was detected by STEREO A at 2024-05-13T12:44Z (see notifications 20240513-AL-006 and 20240513-AL-007) and GOES at 2024-05-13T14:00Z (see notifications 20240513-AL-008 and 20240513-AL-009).\n\nThis SEP event (2024-05-13T18:07:00-SEP-002) is associated with multiple M-class flares from Active Region 13664 (S18W80), including an M1.2 flare with ID 2024-05-13T08:06:00-FLR-001 which peaked at 2024-05-13T08:20Z, an M1.4 flare with ID 2024-05-13T08:23:00-FLR-001 which peaked at 2024-05-13T08:29Z, an M4.9 flare with ID 2024-05-13T08:47:00-FLR-001 which peaked at 2024-05-13T09:33Z, and an M6.6 flare with ID 2024-05-13T09:36:00-FLR-001 which peaked at 2024-05-13T09:44Z (see notifications 20240513-AL-003 and 20240513-AL-004). Also associated with the CME with ID 2024-05-13T09:12:00-CME-001. \n\n"},{"messageType":"SEP","messageID":"20240513-AL-010","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30821/1","messageIssueTime":"2024-05-13T16:33Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP Prediction\n##\n## Message Issue Date: 2024-05-13T16:33:22Z\n## Message ID: 20240513-AL-010\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event forecasted at the orbit of SOHO starting at 2024-05-13T16:19Z.  The flux of one or more of the >15.8 MeV protons channels exceeds 10^(-1) pfu/MeV within next few hours.\n\nNASA spacecraft at the L1 and near-Earth orbits can be impacted.\n\nActivity ID: 2024-05-13T16:19:00-SEP-001.\n\n## Notes: \nEarlier solar energetic particle event prediction by MODEL: REleASE:SOHO/EPHIN 15.8-39.8 MeV with a 2024-05-13T13:10Z event time. \n\nEarlier solar energetic particle event was detected by STEREO A at 2024-05-13T12:44Z (see notifications 20240513-AL-006 and 20240513-AL-007) and GOES at 2024-05-13T14:00Z (see notifications 20240513-AL-008 and 20240513-AL-009).\n\nThis SEP event (2024-05-13T16:19:00-SEP-001) is associated with multiple M-class flares from Active Region 13664 (S17W77), including an M1.2 flare with ID 2024-05-13T08:06:00-FLR-001 which peaked at 2024-05-13T08:20Z, an M1.4 flare with ID 2024-05-13T08:23:00-FLR-001 which peaked at 2024-05-13T08:29Z, an M4.9 flare with ID 2024-05-13T08:47:00-FLR-001 which peaked at 2024-05-13T09:33Z, and an M6.6 flare with ID 2024-05-13T09:36:00-FLR-001 which peaked at 2024-05-13T09:44Z (see notifications 20240513-AL-003 and 20240513-AL-004). Also associated with the CME with ID 2024-05-13T09:12:00-CME-001. \n\n"},{"messageType":"SEP","messageID":"20240513-AL-009","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30819/1","messageIssueTime":"2024-05-13T14:16Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP (GOES)\n##\n## Message Issue Date: 2024-05-13T14:16:34Z\n## Message ID: 20240513-AL-009\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by GOES. The flux of > 10 MeV protons exceeds 10 pfu starting at 2024-05-13T14:00Z.\n\nNASA spacecraft at MEO, GEO and other high-altitude orbits and high-inclination LEO can be impacted.\n\nActivity ID: 2024-05-13T14:00:00-SEP-001.\n\n## Notes: \nEarlier solar energetic particle event was detected by STEREO A at 2024-05-13T12:44Z (see notifications 20240513-AL-006 and 20240513-AL-007).\n\nThis SEP event (2024-05-13T14:00:00-SEP-001) is associated with multiple M-class flares from Active Region 13664 (S18W80), including an M1.2 flare with ID 2024-05-13T08:06:00-FLR-001 which peaked at 2024-05-13T08:20Z, an M1.4 flare with ID 2024-05-13T08:23:00-FLR-001 which peaked at 2024-05-13T08:29Z, an M4.9 flare with ID 2024-05-13T08:47:00-FLR-001 which peaked at 2024-05-13T09:33Z, and an M6.6 flare with ID 2024-05-13T09:36:00-FLR-001 which peaked at 2024-05-13T09:44Z (see notifications 20240513-AL-003 and 20240513-AL-004). Also associated with the CME with ID 2024-05-13T09:12:00-CME-001. \n\n"},{"messageType":"SEP","messageID":"20240513-AL-008","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30818/1","messageIssueTime":"2024-05-13T14:09Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - SEP\n##\n## Message Issue Date: 2024-05-13T14:09:45Z\n## Message ID: 20240513-AL-008\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by GOES.  The flux of > 10 MeV protons exceeds 10 pfu starting at 2024-05-13T14:00Z.\n\nNASA spacecraft at MEO, GEO and other high-altitude orbits and high-inclination LEO can be impacted.\n\nActivity ID: 2024-05-13T14:00:00-SEP-001.\n\n## Notes: \n\n\n\n"},{"messageType":"SEP","messageID":"20240513-AL-007","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30813/1","messageIssueTime":"2024-05-13T13:01Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP (STEREO A)\n##\n## Message Issue Date: 2024-05-13T13:01:26Z\n## Message ID: 20240513-AL-007\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by STEREO A.  The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2024-05-13T12:44Z.\n\nActivity ID: 2024-05-13T12:44:00-SEP-001.\n\n## Notes: \nThis SEP event (2024-05-13T12:44:00-SEP-001) is associated with multiple M-class flares from Active Region 13664 (S18W80), including an M1.2 flare with ID 2024-05-13T08:06:00-FLR-001 which peaked at 2024-05-13T08:20Z, an M1.4 flare with ID 2024-05-13T08:23:00-FLR-001 which peaked at 2024-05-13T08:29Z, an M4.9 flare with ID 2024-05-13T08:47:00-FLR-001 which peaked at 2024-05-13T09:33Z, and an M6.6 flare with ID 2024-05-13T09:36:00-FLR-001 which peaked at 2024-05-13T09:44Z (see notifications 20240513-AL-003 and 20240513-AL-004).\n\nAn associated CME has also been detected in SOHO LASCO images with a plane-of-sky speed of approximately 1200-1400 km/s. Updates will be provided when available.\n\n"},{"messageType":"SEP","messageID":"20240513-AL-006","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30812/1","messageIssueTime":"2024-05-13T12:54Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - SEP\n##\n## Message Issue Date: 2024-05-13T12:54:57Z\n## Message ID: 20240513-AL-006\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by STEREO A.  The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2024-05-13T12:44Z.\n\nActivity ID: 2024-05-13T12:44:00-SEP-001.\n\n## Notes: \n\n\n\n"},{"messageType":"SEP","messageID":"20240513-AL-005","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30810/1","messageIssueTime":"2024-05-13T12:45Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP Prediction\n##\n## Message Issue Date: 2024-05-13T12:45:38Z\n## Message ID: 20240513-AL-005\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event forecasted at the orbit of SOHO starting at 2024-05-13T13:10Z.  The flux of one or more of the >15.8 MeV protons channels exceeds 10^(-1) pfu/MeV within next few hours.\n\nNASA spacecraft at the L1 and near-Earth orbits can be impacted.\n\nActivity ID: 2024-05-13T13:10:00-SEP-001.\n\n## Notes: \n\nThis SEP event (2024-05-13T13:10:00-SEP-001) is associated with multiple M-class flares from Active Region 13664 (S17W77), including an M1.2 flare with ID 2024-05-13T08:06:00-FLR-001 which peaked at 2024-05-13T08:20Z, an M1.4 flare with ID 2024-05-13T08:23:00-FLR-001 which peaked at 2024-05-13T08:29Z, an M4.9 flare with ID 2024-05-13T08:47:00-FLR-001 which peaked at 2024-05-13T09:33Z, and an M6.6 flare with ID 2024-05-13T09:36:00-FLR-001 which peaked at 2024-05-13T09:44Z (see notifications 20240513-AL-003 and 20240513-AL-004).\n\n\n"},{"messageType":"FLR","messageID":"20240513-AL-004","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30805/1","messageIssueTime":"2024-05-13T12:34Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - M6.6 Flare\n##\n## Message Issue Date: 2024-05-13T12:34:53Z\n## Message ID: 20240513-AL-004\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-13T09:36Z. \n\nFlare peak time: 2024-05-13T09:44Z.\n\nFlare intensity: M6.6 class.\n\nSource region: S17W77 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-13T09:36:00-FLR-001.\n\n## Notes: \nLargest peak in a slow, bumpy rise in the x-ray flux from a long-duration eruption from AR 3664. Further analysis is being done on other flare peaks associated with this same eruption in EUV imagery and may include an M1.2, M1.4, and M4.9, peaking at 2024-05-13T08:20Z, 2024-05-13T08:29Z, and 2024-05-13T09:33Z respectively. \n\n\n"},{"messageType":"FLR","messageID":"20240513-AL-003","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30804/1","messageIssueTime":"2024-05-13T09:44Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-13T09:44:01Z\n## Message ID: 20240513-AL-003\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-13T09:38Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"GST","messageID":"20240513-AL-002","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30800/1","messageIssueTime":"2024-05-13T00:53Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-13T00:53:03Z\n## Message ID: 20240513-AL-002\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nOngoing space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 6.33 (moderate) during the synoptic period 2024-05-12T21:00Z to 2024-05-13T00:00Z. \n\nThe storm is likely caused by a prolonged period of negative Bz following the earlier CME arrival around 2024-05-12T08:57Z ( - possibly the arrival of CME with ID 2024-05-09T18:23:00-CME-001 and/or CME with ID 2024-05-10T07:12:00-CME-001 (see notifications 20240509-AL-011, 20240510-AL-003).\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-12T21:00:00-GST-001.\n\n## Notes: \n\n\n"},{"messageType":"GST","messageID":"20240513-AL-001","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30799/1","messageIssueTime":"2024-05-13T00:34Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-13T00:34:53Z\n## Message ID: 20240513-AL-001\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nOngoing space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 6.33 (moderate) during the synoptic period 2024-05-12T21:00Z to 2024-05-13T00:00Z. \n\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-12T21:00:00-GST-001.\n\n## Notes: \n\n\n\n\n"},{"messageType":"CME","messageID":"20240512-AL-004","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30764/1","messageIssueTime":"2024-05-12T17:17Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME Update (Parker Solar Probe, STEREO A)\n##\n## Message Issue Date: 2024-05-12T17:17:09Z\n## Message ID: 20240512-AL-004\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nUpdate on CME with ID 2024-05-11T16:24:00-CME-001 (see previous notification 20240511-AL-017).  Based on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that the CME may impact Parker Solar Probe (glancing blow) and STEREO A (glancing blow).  The flank of the CME may reach Parker Solar Probe at 2024-05-13T08:00Z and STEREO A at 2024-05-14T16:00Z (plus minus 7 hours). \n\n\nUpdated CME parameters are (event downgraded to C-type):\n\nStart time of the event: 2024-05-11T16:24Z.\n\nEstimated speed: ~946 km/s.\n\nEstimated opening half-angle: 25 deg.\n\nDirection (lon./lat.): 53/-2 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-11T16:24:00-CME-001\n\n\nLinks to the movies of the modeled event (includes CME: 2024-05-11T16:24:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_195100_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_195100_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_195100_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_195100_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_195100_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_195100_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_195100_2.0_ENLIL_CONE_STA_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-11T16:24:00-CME-001) is associated with an M8.8 flare from Active Region 13664 (S17W53) which peaked at 2024-05-11T15:25Z with ID 2024-05-11T14:46:00-FLR-001 (see notifications 20240511-AL-014 and 20240511-AL-016).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"FLR","messageID":"20240512-AL-003","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30762/1","messageIssueTime":"2024-05-12T16:37Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X1.0 Flare\n##\n## Message Issue Date: 2024-05-12T16:37:02Z\n## Message ID: 20240512-AL-003\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-12T16:11Z. \n\nFlare peak time: 2024-05-12T16:26Z.\n\nFlare intensity: X1.0 class.\n\nSource region: S21W75 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-12T16:11:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240512-AL-002","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30761/1","messageIssueTime":"2024-05-12T16:25Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-12T16:25:49Z\n## Message ID: 20240512-AL-002\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-12T16:20Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"CME","messageID":"20240512-AL-001","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30758/1","messageIssueTime":"2024-05-12T13:30Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Mars, OSIRIS-APEX, Parker Solar Probe, Solar Orbiter)\n##\n## Message Issue Date: 2024-05-12T13:30:12Z\n## Message ID: 20240512-AL-001\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nC-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-12T03:48Z.\n\nEstimated speed: ~602 km/s.\n\nEstimated opening half-angle: 47 deg.\n\nDirection (lon./lat.): 137/-39 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-12T03:48:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that the CME may impact Mars (glancing blow), OSIRIS-APEX (glancing blow), Parker Solar Probe (glancing blow), and Solar Orbiter (glancing blow).  The flank of the CME may reach Mars at 2024-05-15T22:00Z, OSIRIS-APEX at 2024-05-14T20:00Z, Parker Solar Probe at 2024-05-14T06:00Z, and Solar Orbiter at 2024-05-14T14:00Z (plus minus 7 hours). \n\nLinks to the movies of the modeled event (includes CME: 2024-05-12T03:48:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240512_100900_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240512_100900_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240512_100900_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240512_100900_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240512_100900_2.0_ENLIL_CONE_Mars_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240512_100900_2.0_ENLIL_CONE_SolO_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240512_100900_2.0_ENLIL_CONE_Osiris_timeline.gif\n\n\n## Notes: \n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"CME","messageID":"20240511-AL-017","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30748/1","messageIssueTime":"2024-05-11T20:49Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Parker Solar Probe, STEREO A)\n##\n## Message Issue Date: 2024-05-11T20:49:54Z\n## Message ID: 20240511-AL-017\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nO-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-11T16:24Z.\n\nEstimated speed: ~1088 km/s.\n\nEstimated opening half-angle: 22 deg.\n\nDirection (lon./lat.): 53/-1 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-11T16:24:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that the CME may impact Parker Solar Probe (glancing blow) and STEREO A (glancing blow). The flank of the CME will reach Parker Solar Probe at 2024-05-13T09:00Z and STEREO A at 2024-05-15T15:00Z (plus minus 7 hours). \n\nLinks to the movies of the modeled event (includes CME: 2024-05-11T16:24:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_193500_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_193500_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_193500_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_193500_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_193500_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_193500_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_193500_2.0_ENLIL_CONE_STA_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-11T16:24:00-CME-001) is associated with M8.8 flare from AR 3664 (S17W53) with ID 2024-05-11T14:46:00-FLR-001 which peaked at 2024-05-11T15:25Z (see notifications 20240511-AL-014, 20240511-AL-016).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"FLR","messageID":"20240511-AL-016","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30732/1","messageIssueTime":"2024-05-11T15:41Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - M8.8 Flare\n##\n## Message Issue Date: 2024-05-11T15:41:50Z\n## Message ID: 20240511-AL-016\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-11T14:46Z. \n\nFlare peak time: 2024-05-11T15:25Z.\n\nFlare intensity: M8.8 class.\n\nSource region: S17W53 (Active Region 13664) (based on SDO imagery).\n\nOngoing elevation in energetic proton fluxes may be enhanced by this event. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-11T14:46:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"GST","messageID":"20240511-AL-015","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30731/1","messageIssueTime":"2024-05-11T15:14Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-11T15:14:04Z\n## Message ID: 20240511-AL-015\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nIntensifying space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 9 (extreme) during the synoptic period 2024-05-11T09:00Z to 2024-05-11T12:00Z. \n\nThe storm is caused by the Interplanetary Shock with ID 2024-05-10T21:39:00-IPS-001 (see notification 20240510-AL-017) and the earlier Interplanetary Shock with ID 2024-05-10T16:36:00-IPS-001 (see notification 20240510-AL-010) which are associated with the arrivals of CME with ID 2024-05-08T05:36:00-CME-001 (see notifications 20240508-AL-012, 20240509-AL-010), CME with ID 2024-05-08T12:24:00-CME-001 (see notifications 20240508-AL-009, 20240509-AL-010), CME with ID 2024-05-08T22:24:00-CME-001 (see notifications 20240509-AL-009, 20240509-AL-010) and/or possibly CME with ID 2024-05-09T09:24:00-CME-001 (see notifications 20240509-AL-006, 20240509-AL-010).\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-10T15:00:00-GST-001.\n\n## Notes: \nThis event is also associated with modeled Magnetopause Crossing with ID 2024-05-10T18:01:00-MPC-001 (see notifications 20240510-AL-011, 20240510-AL-012 and 20240511-AL-001).\n\n\n\n"},{"messageType":"FLR","messageID":"20240511-AL-014","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30730/1","messageIssueTime":"2024-05-11T15:13Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-11T15:13:30Z\n## Message ID: 20240511-AL-014\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-11T15:09Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"SEP","messageID":"20240511-AL-013","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30728/1","messageIssueTime":"2024-05-11T15:03Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP (STEREO A)\n##\n## Message Issue Date: 2024-05-11T15:03:54Z\n## Message ID: 20240511-AL-013\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by STEREO A.  The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2024-05-11T04:07Z.\n\nActivity ID: 2024-05-11T04:07:00-SEP-001.\n\n## Notes: \n\nThis SEP event (2024-05-11T04:07:00-SEP-001) is associated with X5.8 flare from Active Region 3664 (S17W47) with ID 2024-05-11T01:10:00-FLR-001 which peaked at 2024-05-11T01:23Z (see notifications 20240511-AL-004, 20240511-AL-005) and O-Type CME with ID 2024-05-11T01:36:00-CME-001 (see notifications 20240511-AL-009, 20240511-AL-012).\n\nThe flux of 13-100 MeV protons had previously exceeded 10^(-1) pfu/MeV starting at 2024-05-10T14:50Z (SEP event with ID 2024-05-10T14:50:00-SEP-001, see notifications 20240510-AL-008, 20240510-AL-009) in association with numerous M and X-class flares from Active Region 13664 and associated CMEs from 2024-05-08 and 2024-05-09. The 13-100 MeV protons flux dipped below 10^(-1) pfu/MeV pfu after a STEREO data gap spanning 2024-05-10T21:08Z to 2024-05-11T01:35Z, and has again risen above the threshold of 10^(-1) pfu/MeV starting at 2024-05-11T04:07Z.\n\n\n"},{"messageType":"CME","messageID":"20240511-AL-012","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30727/1","messageIssueTime":"2024-05-11T14:23Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME update (Lucy, Mars, Parker Solar Probe, STEREO A, OSIRIS-APEX, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-11T14:23:10Z\n## Message ID: 20240511-AL-012\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nUpdate on CME with ID 2024-05-11T01:36:00-CME-001 (see previous notification 20240511-AL-009). Based on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Lucy, Mars, Parker Solar Probe, STEREO A, and OSIRIS-APEX (glancing blow). The leading edge of the CME will reach Lucy at 2024-05-14T18:37Z, Mars at 2024-05-13T17:42Z, Parker Solar Probe at 2024-05-12T05:42Z, STEREO A at 2024-05-12T20:25Z (plus minus 7 hours), and the flank of the CME will reach OSIRIS-APEX at 2024-05-13T04:00Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-13T04:59Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 5-7 (minor to strong).\n   \n\nUpdated CME parameters are (event remains to O-type):\n\nStart time of the event: 2024-05-11T01:36Z.\n\nEstimated speed: ~1263 km/s.\n\nEstimated opening half-angle: 51 deg.\n\nDirection (lon./lat.): 51/0 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-11T01:36:00-CME-001\n\n\nLinks to the movies of the modeled event (includes CME: 2024-05-11T01:36:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_ENLIL_CONE_STA_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_ENLIL_CONE_Lucy_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_ENLIL_CONE_Mars_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240511_042200_2.0_ENLIL_CONE_Osiris_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-11T01:36:00-CME-001) is associated with X5.8 flare from Active Region 3664 (S17W47) with ID 2024-05-11T01:10:00-FLR-001 which peaked at 2024-05-11T01:23Z (see notifications 20240511-AL-004, 20240511-AL-005) and SEP at GOES-P with ID 2024-05-11T02:10:00-SEP-001 (see notifications 20240511-AL-006, 20240511-AL-007).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"FLR","messageID":"20240511-AL-011","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30724/1","messageIssueTime":"2024-05-11T12:33Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X1.5 Flare\n##\n## Message Issue Date: 2024-05-11T12:33:23Z\n## Message ID: 20240511-AL-011\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-11T11:15Z. \n\nFlare peak time: 2024-05-11T11:44Z.\n\nFlare intensity: X1.5 class.\n\nSource region: S19W60 (Active Region 13664) (based on SDO imagery).\n\nOngoing elevation in energetic proton fluxes may be enhanced by this event. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-11T11:15:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240511-AL-010","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30723/1","messageIssueTime":"2024-05-11T11:37Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-11T11:37:27Z\n## Message ID: 20240511-AL-010\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-11T11:31Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"CME","messageID":"20240511-AL-009","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30721/1","messageIssueTime":"2024-05-11T04:50Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME\n##\n## Message Issue Date: 2024-05-11T04:50:13Z\n## Message ID: 20240511-AL-009\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nO-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-11T01:36Z.\n\nEstimated speed: ~1372 km/s.\n\nEstimated opening half-angle: 49 deg.\n\nDirection (lon./lat.): 47/-1 in Heliocentric Earth Equatorial coordinates.\n\nNASA spacecraft near Earth and between Earth and Mars can be affected.  \n\nThe above parameters are preliminary, the CME is still being analyzed and updates will be provided when available. \n\nActivity ID: 2024-05-11T01:36:00-CME-001\n\n## Notes: \n\nThis CME event (2024-05-11T01:36:00-CME-001) is associated with X5.8 flare from Active Region 3664 (S17W47) with ID 2024-05-11T01:10:00-FLR-001 which peaked at 2024-05-11T01:23Z (see notifications 20240511-AL-004, 20240511-AL-005) and SEP at GOES-P with ID 2024-05-11T02:10:00-SEP-001 (see notifications 20240511-AL-006, 20240511-AL-007).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"SEP","messageID":"20240511-AL-008","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30718/1","messageIssueTime":"2024-05-11T04:13Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - SEP\n##\n## Message Issue Date: 2024-05-11T04:13:59Z\n## Message ID: 20240511-AL-008\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by STEREO A.  The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2024-05-11T04:07Z.\n\nActivity ID: 2024-05-11T04:07:00-SEP-001.\n\n## Notes: \n\n\n\n"},{"messageType":"SEP","messageID":"20240511-AL-007","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30716/1","messageIssueTime":"2024-05-11T02:46Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP\n##\n## Message Issue Date: 2024-05-11T02:46:21Z\n## Message ID: 20240511-AL-007\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by GOES.  The flux of > 100 MeV protons exceeds 1 pfu starting at 2024-05-11T02:10Z.\n\nNASA Spacecraft at MEO, GEO and other high-altitude orbits and high-inclination LEO can be impacted.\n\nActivity ID: 2024-05-11T02:10:00-SEP-001.\n\n## Notes: \n\nThis SEP event (2024-05-11T02:10:00-SEP-001) is associated with X5.8 flare from Active Region 3664 (S17W47) with ID 2024-05-11T01:10:00-FLR-001 which peaked at 2024-05-11T01:23Z (see notifications 20240511-AL-004, 20240511-AL-005) and an associated partial halo CME that is currently being analyzed.\n\nThe flux of > 10 MeV protons had previously exceeded 10 pfu starting at 2024-05-10T13:35Z (SEP event with ID 2024-05-10T13:35:00-SEP-001, see notifications 20240510-AL-004, 20240510-AL-005) in association with numerous M and X-class flares from Active Region 13664 and associated CMEs from 2024-05-08 and 2024-05-09. The > 10 MeV proton flux dipped just below 10 pfu at 2024-05-11T01:10Z and has again risen above the threshold of 10 pfu at 2024-05-11T02:10Z.\n\n\n"},{"messageType":"SEP","messageID":"20240511-AL-006","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30715/1","messageIssueTime":"2024-05-11T02:30Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - SEP\n##\n## Message Issue Date: 2024-05-11T02:30:46Z\n## Message ID: 20240511-AL-006\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by GOES.  The flux of > 100 MeV protons exceeds 1 pfu starting at 2024-05-11T02:10Z.\n\nNASA Spacecraft at MEO, GEO and other high-altitude orbits and high-inclination LEO can be impacted.\n\nActivity ID: 2024-05-11T02:10:00-SEP-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240511-AL-005","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30713/1","messageIssueTime":"2024-05-11T01:49Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X5.8 Flare\n##\n## Message Issue Date: 2024-05-11T01:49:36Z\n## Message ID: 20240511-AL-005\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-11T01:10Z. \n\nFlare peak time: 2024-05-11T01:23Z.\n\nFlare intensity: X5.8 class.\n\nSource region: S17W47  (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-11T01:10:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240511-AL-004","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30712/1","messageIssueTime":"2024-05-11T01:27Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-11T01:27:17Z\n## Message ID: 20240511-AL-004\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-11T01:15Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"GST","messageID":"20240511-AL-003","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30708/1","messageIssueTime":"2024-05-11T00:39Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-11T00:39:58Z\n## Message ID: 20240511-AL-003\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nIntensifying space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 9 (extreme) during the synoptic period 2024-05-10T21:00Z to 2024-05-11T00:00Z. \n\nThe storm is caused by the Interplanetary Shock with ID 2024-05-10T21:39:00-IPS-001 (see notification 20240510-AL-017) and the earlier Interplanetary Shock with ID 2024-05-10T16:36:00-IPS-001 (see notification 20240510-AL-010) which are associated with the arrivals of CME with ID 2024-05-08T05:36:00-CME-001 (see notifications 20240508-AL-012, 20240509-AL-010), CME with ID 2024-05-08T12:24:00-CME-001 (see notifications 20240508-AL-009, 20240509-AL-010), CME with ID 2024-05-08T22:24:00-CME-001 (see notifications 20240509-AL-009, 20240509-AL-010) and/or possibly CME with ID 2024-05-09T09:24:00-CME-001 (see notifications 20240509-AL-006, 20240509-AL-010).\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-10T15:00:00-GST-001.\n\n## Notes: \nThis event is also associated with modeled Magnetopause Crossing with ID 2024-05-10T18:01:00-MPC-001 (see notifications 20240510-AL-011, 20240510-AL-012 and 20240511-AL-001).\n\n\n"},{"messageType":"GST","messageID":"20240511-AL-002","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30707/1","messageIssueTime":"2024-05-11T00:34Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-11T00:34:33Z\n## Message ID: 20240511-AL-002\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nIntensifying space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 9 (extreme) during the synoptic period 2024-05-10T21:00Z to 2024-05-11T00:00Z. \n\nThe storm is caused by CME with ID 2024-05-08T05:36:00-CME-001 (see notification(s) 20240508-AL-012, 20240509-AL-010), CME with ID 2024-05-08T12:24:00-CME-001 (see notification(s) 20240508-AL-009, 20240509-AL-010), CME with ID 2024-05-08T22:24:00-CME-001 (see notification(s) 20240509-AL-009, 20240509-AL-010) and CME with ID 2024-05-09T09:24:00-CME-001 (see notification(s) 20240509-AL-006, 20240509-AL-010).\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-10T15:00:00-GST-001.\n\n## Notes: \n\n\n\n\n"},{"messageType":"MPC","messageID":"20240511-AL-001","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30706/1","messageIssueTime":"2024-05-11T00:12Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Magnetopause Crossing\n##\n## Message Issue Date: 2024-05-11T00:12:51Z\n## Message ID: 20240511-AL-001\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nStrong compression of the magnetosphere continues. Simulations carried out at NASA Community Coordinated Modeling Center indicate that the magnetopause separating magnetospheric and solar wind plasma has been intermittently close to the geosynchronous orbit since 2024-05-10T18:01Z, after the first Interplanetary Shock of today with ID 2024-05-10T16:36:00-IPS-001 (see notifications 20240510-AL-010, 20240510-AL-011, 20240510-AL-012). \n\nAccording to the simulations, the magnetopause is currently close to the geosynchronous orbit following the second Interplanetary Shock with ID 2024-05-10T21:39:00-IPS-001 (see notification 20240510-AL-017). \n\nThe activity is associated with the arrival of CME with ID 2024-05-08T05:36:00-CME-001 (see notifications 20240508-AL-012, 20240509-AL-010), CME with ID 2024-05-08T12:24:00-CME-001 (see notifications 20240508-AL-009, 20240509-AL-010), CME with ID 2024-05-08T22:24:00-CME-001 (see notifications 20240509-AL-009, 20240509-AL-010) and/or CME with ID 2024-05-09T09:24:00-CME-001 (see notifications 20240509-AL-006, 20240509-AL-010).\n\nNASA spacecraft at the geosynchronous orbits may be exposed to solar wind plasma and magnetic field conditions.\n\nActivity ID: 2024-05-10T18:01:00-MPC-001.\n\n## Notes \n\n\n"},{"messageType":"IPS","messageID":"20240510-AL-017","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30705/1","messageIssueTime":"2024-05-10T22:24Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Interplanetary Shock\n##\n## Message Issue Date: 2024-05-10T22:24:26Z\n## Message ID: 20240510-AL-017\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant interplanetary shock detected by DSCOVR at L1 at 2024-05-10T21:39Z. \n\nThe shock is likely caused by the arrival of CME with ID 2024-05-08T22:24:00-CME-001 (see notifications 20240509-AL-009, 20240509-AL-010) and/or CME with ID 2024-05-09T09:24:00-CME-001 (see notifications 20240509-AL-006, 20240509-AL-010). \n\nStrong magnetospheric compression and geomagnetic storm expected.\n\nActivity ID: 2024-05-10T21:39:00-IPS-001.\n\n## Notes: \nThis shock is following on the heels of another shock earlier today with ID 2024-05-10T16:36:00-IPS-001 (see notification 20240510-AL-010). The attribution of these two shocks to CMEs is still in progress and updates will be provided when available.\n\n\n"},{"messageType":"GST","messageID":"20240510-AL-016","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30703/1","messageIssueTime":"2024-05-10T22:01Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-10T22:01:15Z\n## Message ID: 20240510-AL-016\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nIntensifying space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 8.67 (severe) during the synoptic period 2024-05-10T18:00Z to 2024-05-10T21:00Z. \n\nThe storm is caused by the Interplanetary Shock with ID 2024-05-10T16:36:00-IPS-001 (see notification 20240510-AL-010) which is associated with the arrival of one or more of the following CMEs: CME with ID 2024-05-08T05:36:00-CME-001 (see notifications 20240508-AL-012, 20240509-AL-010), CME with ID 2024-05-08T12:24:00-CME-001 (see notifications 20240508-AL-009, 20240509-AL-010) and/or possibly CMEs with ID 2024-05-08T22:24:00-CME-001 (see notifications 20240509-AL-009, 20240509-AL-010) and 2024-05-09T09:24:00-CME-001 (see notifications 20240509-AL-006, 20240509-AL-010). \n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-10T15:00:00-GST-001.\n\n## Notes: \nThis event is also associated with modeled Magnetopause Crossing with ID 2024-05-10T18:01:00-MPC-001 (see notifications 20240510-AL-011 and 20240510-AL-012).\n\n\n"},{"messageType":"GST","messageID":"20240510-AL-015","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30702/1","messageIssueTime":"2024-05-10T21:35Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-10T21:35:45Z\n## Message ID: 20240510-AL-015\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nIntensifying space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 8.67 (severe) during the synoptic period 2024-05-10T18:00Z to 2024-05-10T21:00Z. \n\nThe storm is caused by CME with ID 2024-05-07T03:12:00-CME-001, CME with ID 2024-05-07T05:24:00-CME-001 and CME with ID 2024-05-08T05:36:00-CME-001 (see notification(s) 20240508-AL-012, 20240509-AL-010).\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-10T15:00:00-GST-001.\n\n## Notes: \n\n\n\n\n"},{"messageType":"GST","messageID":"20240510-AL-014","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30695/1","messageIssueTime":"2024-05-10T19:19Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-10T19:19:23Z\n## Message ID: 20240510-AL-014\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nOngoing space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 7.67 (severe) during the synoptic period 2024-05-10T15:00Z to 2024-05-10T18:00Z. \n\nThe storm is caused by the Interplanetary Shock with ID 2024-05-10T16:36:00-IPS-001 (see notification 20240510-AL-010) which is associated with the arrival of the CME with ID 2024-05-07T03:12:00-CME-001, CME with ID 2024-05-07T05:24:00-CME-001, and/or CME with ID 2024-05-08T05:36:00-CME-001 (see notifications 20240508-AL-012 and 20240509-AL-010).\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-10T15:00:00-GST-001.\n\n## Notes: \n\nThis event is also associated with modeled Magnetopause Crossing with ID 2024-05-10T18:01:00-MPC-001 (see notifications 20240510-AL-011 and 20240510-AL-012).\n\n\n"},{"messageType":"GST","messageID":"20240510-AL-013","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30694/1","messageIssueTime":"2024-05-10T18:44Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Geomagnetic Storm\n##\n## Message Issue Date: 2024-05-10T18:44:21Z\n## Message ID: 20240510-AL-013\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nOngoing space weather storm in the Earth's magnetosphere. Geomagnetic Kp index has reached level 7.67 (severe) during the synoptic period 2024-05-10T15:00Z to 2024-05-10T18:00Z. \n\n\nNASA spacecraft at GEO, MEO, polar and other orbits passing through or in the vicinity of the Earth's ring current and auroral regions can be impacted.\n\nActivity ID: 2024-05-10T15:00:00-GST-001.\n\n## Notes: \n\n\n\n\n"},{"messageType":"MPC","messageID":"20240510-AL-012","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30692/1","messageIssueTime":"2024-05-10T17:39Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Magnetopause Crossing\n##\n## Message Issue Date: 2024-05-10T17:39:02Z\n## Message ID: 20240510-AL-012\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nStrong compression of the magnetosphere detected. Simulations carried out at NASA Community Coordinated Modeling Center indicate that the magnetopause separating magnetospheric and solar wind plasma is close to the geosynchronous orbit starting at 2024-05-10T18:01Z.\n\nThe activity is associated with the Interplanetary Shock with ID 2024-05-10T16:36:00-IPS-001 (see notification 20240510-AL-010) which is associated with the arrival of the CME with ID 2024-05-07T03:12:00-CME-001, CME with ID 2024-05-07T05:24:00-CME-001, and/or CME with ID 2024-05-08T05:36:00-CME-001 (see notifications 20240508-AL-012 and 20240509-AL-010).\n\nNASA spacecraft at the geosynchronous orbits may be exposed to solar wind plasma and magnetic field conditions.\n\nActivity ID: 2024-05-10T18:01:00-MPC-001.\n\n## Notes \n\n\n\n"},{"messageType":"MPC","messageID":"20240510-AL-011","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30691/1","messageIssueTime":"2024-05-10T17:33Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Magnetopause Crossing\n##\n## Message Issue Date: 2024-05-10T17:33:04Z\n## Message ID: 20240510-AL-011\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nStrong compression of the magnetosphere detected. Simulations carried out at NASA Community Coordinated Modeling Center indicate that the magnetopause separating magnetospheric and solar wind plasma is close to the geosynchronous orbit starting at 2024-05-10T18:01Z.\n\n\nNASA spacecraft at the geosynchronous orbits may be exposed to solar wind plasma and magnetic field conditions.\n\nActivity ID: 2024-05-10T18:01:00-MPC-001.\n\n## Notes \n\n\n\n"},{"messageType":"IPS","messageID":"20240510-AL-010","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30689/1","messageIssueTime":"2024-05-10T17:01Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - Interplanetary Shock\n##\n## Message Issue Date: 2024-05-10T17:01:00Z\n## Message ID: 20240510-AL-010\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant interplanetary shock detected by ACE at L1 at 2024-05-10T16:36Z. \n\nThe shock is likely caused by the CME with ID 2024-05-07T03:12:00-CME-001, CME with ID 2024-05-07T05:24:00-CME-001 and/or CME with ID 2024-05-08T05:36:00-CME-001 (see notifications 20240508-AL-012 and 20240509-AL-010).\n\nStrong magnetospheric compression and geomagnetic storm expected. This arrival signature is still developing and analysis is ongoing.\n\nActivity ID: 2024-05-10T16:36:00-IPS-001.\n\n## Notes: \n\n\n\n"},{"messageType":"SEP","messageID":"20240510-AL-009","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30686/1","messageIssueTime":"2024-05-10T15:17Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP (STEREO A)\n##\n## Message Issue Date: 2024-05-10T15:17:04Z\n## Message ID: 20240510-AL-009\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by STEREO A.  The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2024-05-10T14:50Z.\n\nActivity ID: 2024-05-10T14:50:00-SEP-001.\n\n## Notes: \n\nThis SEP event (2024-05-10T13:35:00-SEP-001) is associated with numerous M and X-class flares from Active Region 13664 and associated CMEs starting as early as 2024-05-08. Main contributors include: the M3.5 flare and X1.0 flare associated with the CME with ID 2024-05-08T05:36:00-CME-001; the M8.6 flare associated with the CME with ID 2024-05-08T12:24:00-CME-001; the X1.0 flare and M9.8 flare associated with the CME with ID 2024-05-08T22:24:00-CME-001; the X2.2 flare associated with the CME with ID 2024-05-09T09:24:00-CME-001; the X1.1 flare associated with the CME with ID 2024-05-09T18:23:00-CME-001; and the X3.9 flare associated with the CME with ID 2024-05-10T07:12:00-CME-001.\n\n\n"},{"messageType":"SEP","messageID":"20240510-AL-008","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30685/1","messageIssueTime":"2024-05-10T15:03Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - SEP\n##\n## Message Issue Date: 2024-05-10T15:03:50Z\n## Message ID: 20240510-AL-008\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by STEREO A.  The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2024-05-10T14:50Z.\n\nActivity ID: 2024-05-10T14:50:00-SEP-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240510-AL-007","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30682/1","messageIssueTime":"2024-05-10T14:28Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - M5.9 Flare\n##\n## Message Issue Date: 2024-05-10T14:28:15Z\n## Message ID: 20240510-AL-007\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-10T13:58Z. \n\nFlare peak time: 2024-05-10T14:11Z.\n\nFlare intensity: M5.9 class.\n\nSource region: S16W40 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-10T13:58:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240510-AL-006","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30681/1","messageIssueTime":"2024-05-10T14:15Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-10T14:15:08Z\n## Message ID: 20240510-AL-006\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-10T14:08Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"SEP","messageID":"20240510-AL-005","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30679/1","messageIssueTime":"2024-05-10T14:12Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP (GOES, SOHO)\n##\n## Message Issue Date: 2024-05-10T14:12:13Z\n## Message ID: 20240510-AL-005\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by GOES and SOHO. At GOES, the flux of > 10 MeV protons exceeds 10 pfu starting at 2024-05-10T13:35Z.\n\nThe flux of one or more of the >15.8 MeV protons channels exceeds 10^(-1) pfu/MeV starting at 2024-05-10T12:59Z.\n\nNASA spacecraft at MEO, GEO and other high-altitude orbits and high-inclination LEO can be impacted.\n\nActivity ID: 2024-05-10T13:35:00-SEP-001.\n\n## Notes: \n\nThis SEP event (2024-05-10T13:35:00-SEP-001) is associated with numerous M and X-class flares from Active Region 13664 and associated CMEs starting as early as 2024-05-08. Main contributors include: the M3.5 flare and X1.0 flare associated with the CME with ID 2024-05-08T05:36:00-CME-001; the M8.6 flare associated with the CME with ID 2024-05-08T12:24:00-CME-001; the X1.0 flare and M9.8 flare associated with the CME with ID 2024-05-08T22:24:00-CME-001; the X2.2 flare associated with the CME with ID 2024-05-09T09:24:00-CME-001; the X1.1 flare associated with the CME with ID 2024-05-09T18:23:00-CME-001; and the X3.9 flare associated with the CME with ID 2024-05-10T07:12:00-CME-001.\n\n\n"},{"messageType":"SEP","messageID":"20240510-AL-004","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30678/1","messageIssueTime":"2024-05-10T13:46Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - SEP\n##\n## Message Issue Date: 2024-05-10T13:46:58Z\n## Message ID: 20240510-AL-004\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event detected by GOES.  The flux of > 10 MeV protons exceeds 10 pfu starting at 2024-05-10T13:35Z.\n\nNASA spacecraft at MEO, GEO and other high-altitude orbits and high-inclination LEO can be impacted.\n\nActivity ID: 2024-05-10T13:35:00-SEP-001.\n\n## Notes: \n\n\n\n"},{"messageType":"CME","messageID":"20240510-AL-003","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30674/1","messageIssueTime":"2024-05-10T13:38Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Lucy, STEREO A, Parker Solar Probe, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-10T13:38:36Z\n## Message ID: 20240510-AL-003\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nO-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-10T07:12Z.\n\nEstimated speed: ~1018 km/s.\n\nEstimated opening half-angle: 41 deg.\n\nDirection (lon./lat.): 31/-2 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-10T07:12:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Lucy, STEREO A, and Parker Solar Probe (glancing blow).  The leading edge or flank of the CME may reach Lucy at 2024-05-14T12:28Z, STEREO A at 2024-05-12T07:16Z, and Parker Solar Probe at 2024-05-12T02:00Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-12T14:00Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 5-7 (minor to strong).\n   \n  \nLinks to the movies of the modeled event (includes CME: 2024-05-10T07:12:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240510_103500_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240510_103500_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240510_103500_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240510_103500_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240510_103500_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240510_103500_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240510_103500_2.0_ENLIL_CONE_STA_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-10T07:12:00-CME-001) is associated with X3.9 flare from Active Region 13664 (S18W37) with ID 2024-05-10T06:27:00-FLR-001 which peaked at 2024-05-10T06:54Z (see notifications 20240510-AL-001 and 20240510-AL-002).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"FLR","messageID":"20240510-AL-002","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30668/1","messageIssueTime":"2024-05-10T11:37Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X3.9 Flare\n##\n## Message Issue Date: 2024-05-10T11:37:53Z\n## Message ID: 20240510-AL-002\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-10T06:27Z. \n\nFlare peak time: 2024-05-10T06:54Z.\n\nFlare intensity: X3.9 class.\n\nSource region: S18W37 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-10T06:27:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240510-AL-001","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30667/1","messageIssueTime":"2024-05-10T06:51Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-10T06:51:02Z\n## Message ID: 20240510-AL-001\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-10T06:41Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"CME","messageID":"20240509-AL-011","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30662/1","messageIssueTime":"2024-05-09T23:35Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Lucy, STEREO A, Parker Solar Probe, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-09T23:35:58Z\n## Message ID: 20240509-AL-011\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nC-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-09T18:23Z.\n\nEstimated speed: ~895 km/s.\n\nEstimated opening half-angle: 44 deg.\n\nDirection (lon./lat.): 30/-6 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-09T18:23:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Lucy, STEREO A, and Parker Solar Probe (glancing blow).  The leading edge or flank of the CME will reach Lucy at 2024-05-13T03:24Z, STEREO A at 2024-05-11T01:31Z, and Parker Solar Probe at 2024-05-10T21:00Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-11T07:55Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 5-7 (minor to strong).\n   \n  \nLinks to the movies of the modeled event (includes CME: 2024-05-09T18:23:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_02:500_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_02:500_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_02:500_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_02:500_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_02:500_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_02:500_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_02:500_2.0_ENLIL_CONE_STA_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-09T18:23:00-CME-001) is associated with X1.1 flare from Active Region 3664 (S18W29) with ID 2024-05-09T17:23:00-FLR-001 which peaked at 2024-05-09T17:44Z (see notifications 20240509-AL-007, 20240509-AL-008).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"CME","messageID":"20240509-AL-010","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30653/1","messageIssueTime":"2024-05-09T21:24Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CMEs update (Psyche, Lucy, STEREO A, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-09T21:24:51Z\n## Message ID: 20240509-AL-010\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nUpdate on CMEs with IDs 2024-05-08T05:36:00-CME-001 (see previous notification 20240508-AL-012), 2024-05-08T12:24:00-CME-001 (see previous notification 20240508-AL-009), 2024-05-08T19:12:00-CME-001 (see previous notification 20240509-AL-005), 2024-05-08T22:24:00-CME-001 (see previous notification 20240509-AL-009), and 2024-05-09T09:24:00-CME-001 (see previous notification 20240509-AL-006).  Based on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that the CMEs may affect Psyche (glancing blow), Lucy, and STEREO A.  The flank of the CMEs will reach Psyche at 2024-05-16T00:00Z and the combined leading edge of the CMEs will reach Lucy at 2024-05-12T04:05Z and STEREO A at 2024-05-10T07:53Z (plus minus 7 hours).\n \nThe simulation also indicates that the CMEs may impact NASA missions near Earth. Simulations indicate that the combined leading edge of the CMEs will reach NASA missions near Earth at about 2024-05-10T13:03Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 8-9 (severe to extreme).\n\nCME parameters are (C-type):\n\n1: Start time of the event: 2024-05-08T05:36Z.\n\nEstimated speed: ~870 km/s.\n\nEstimated opening half-angle: 43 deg.\n\nDirection (lon./lat.): 9/-7 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T05:36:00-CME-001\n\n\n2: Start time of the event: 2024-05-08T12:24Z.\n\nEstimated speed: ~776 km/s.\n\nEstimated opening half-angle: 45 deg.\n\nDirection (lon./lat.): 3/-5 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T12:24:00-CME-001\n\n\n3: Start time of the event: 2024-05-08T19:12Z.\n\nEstimated speed: ~828 km/s.\n\nEstimated opening half-angle: 38 deg.\n\nDirection (lon./lat.): -23/3 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T19:12:00-CME-001\n\n\n4: Start time of the event: 2024-05-08T22:24Z.\n\nEstimated speed: ~1130 km/s.\n\nEstimated opening half-angle: 40 deg.\n\nDirection (lon./lat.): 12/-16 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T22:24:00-CME-001\n\n\n5: Start time of the event: 2024-05-09T09:24Z.\n\nEstimated speed: ~1330 km/s.\n\nEstimated opening half-angle: 45 deg.\n\nDirection (lon./lat.): 19/-6 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-09T09:24:00-CME-001\n\n\nLinks to the movies of the modeled event (includes CMEs: 2024-05-08T05:36:00-CME-001, 2024-05-08T12:24:00-CME-001, 2024-05-08T19:12:00-CME-001, 2024-05-08T22:24:00-CME-001, 2024-05-09T09:24:00-CME-001):\n\n(a) 2 AU outer boundary\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_2.0_ENLIL_CONE_STA_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_2.0_ENLIL_CONE_Lucy_timeline.gif\n\n(b) 5.5 AU outer boundary\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_5.5_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_5.5_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093200_5.5_ENLIL_CONE_Psyche_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-08T05:36:00-CME-001) is associated with the M3.5 flare from AR13664 (S21W10) with ID 2024-05-08T04:20:00-FLR-001 which peaked at 2024-05-08T04:30Z and  the X1.0 flare from AR13664 (S22W10) with ID 2024-05-08T04:37:00-FLR-001 which peaked at 2024-05-08T05:09Z (see notifications 20240508-AL-003, 20240508-AL-006).\n\nThis CME event (2024-05-08T12:24:00-CME-001) is associated with the M8.6 flare from AR13664 (S20W11) with ID 2024-05-08T11:26:00-FLR-001 which peaked at 2024-05-08T12:04Z (see notifications 20240508-AL-005, 20240508-AL-007).\n\nThis CME event (2024-05-08T22:24:00-CME-001) is associated with the X1.0 flare from AR13664 (S20W17) with ID 2024-05-08T21:08:00-FLR-001 which peaked at 2024-05-08T21:40Z (see notifications 20240508-AL-013, 20240508-AL-014) and M9.8 flare from AR13664 (S22W22) with ID 2024-05-08T22:05:00-FLR-001 which peaked at 2024-05-08T22:27Z (see notification 20240509-AL-003).\n\nThis CME event (2024-05-09T09:24:00-CME-001) is associated with the X2.2 flare from AR13664 (S20W25) with ID 2024-05-09T08:45:00-FLR-001 which peaked at 2024-05-09T09:13Z (see notifications 20240509-AL-001, 20240509-AL-002).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"CME","messageID":"20240509-AL-009","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30649/1","messageIssueTime":"2024-05-09T20:03Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Lucy, STEREO A, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-09T20:03:35Z\n## Message ID: 20240509-AL-009\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nO-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-08T22:24Z.\n\nEstimated speed: ~1130 km/s.\n\nEstimated opening half-angle: 40 deg.\n\nDirection (lon./lat.): 12/-16 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T22:24:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Lucy and STEREO A.  The leading edge of the CME will reach Lucy at 2024-05-12T18:10Z and STEREO A at 2024-05-10T19:07Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-10T23:46Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 6-8 (moderate to severe).\n   \n  \nLinks to the movies of the modeled event (includes CME: 2024-05-08T22:24:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_014300_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_014300_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_014300_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_014300_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_014300_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_014300_2.0_ENLIL_CONE_STA_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-08T22:24:00-CME-001) is associated with the X1.0 flare from AR13664 (S20W17) with ID 2024-05-08T21:08:00-FLR-001 which peaked at 2024-05-08T21:40Z (see notifications 20240508-AL-013, 20240508-AL-014) and M9.8 flare from AR13664 (S22W22) with ID 2024-05-08T22:05:00-FLR-001 which peaked at 2024-05-08T22:27Z (see notification 20240509-AL-003).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"FLR","messageID":"20240509-AL-008","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30636/1","messageIssueTime":"2024-05-09T17:54Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X1.1 Flare\n##\n## Message Issue Date: 2024-05-09T17:54:32Z\n## Message ID: 20240509-AL-008\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-09T17:23Z. \n\nFlare peak time: 2024-05-09T17:44Z.\n\nFlare intensity: X1.1 class.\n\nSource region: S18W29 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-09T17:23:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240509-AL-007","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30635/1","messageIssueTime":"2024-05-09T17:42Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-09T17:42:53Z\n## Message ID: 20240509-AL-007\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-09T17:33Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"CME","messageID":"20240509-AL-006","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30628/1","messageIssueTime":"2024-05-09T17:04Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Lucy, STEREO A, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-09T17:04:16Z\n## Message ID: 20240509-AL-006\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nO-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-09T09:24Z.\n\nEstimated speed: ~1330 km/s.\n\nEstimated opening half-angle: 45 deg.\n\nDirection (lon./lat.): 19/-6 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-09T09:24:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Lucy and STEREO A.  The leading edge of the CME will reach Lucy at 2024-05-12T21:29Z and STEREO A at 2024-05-11T01:10Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-11T05:02Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 6-8 (moderate to severe).\n   \n  \nLinks to the movies of the modeled event (includes CME: 2024-05-09T09:24:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_115600_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_115600_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_115600_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_115600_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_115600_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240509_115600_2.0_ENLIL_CONE_STA_timeline.gif\n\n\n## Notes: \n\nThis CME event (2024-05-09T09:24:00-CME-001) is associated with the X2.2 flare from AR13664 (S20W25) with ID 2024-05-09T08:45:00-FLR-001 which peaked at 2024-05-09T09:13Z (see notifications 20240509-AL-001, 20240509-AL-002).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"CME","messageID":"20240509-AL-005","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30624/1","messageIssueTime":"2024-05-09T16:39Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Psyche, STEREO A, Lucy, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-09T16:39:40Z\n## Message ID: 20240509-AL-005\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nC-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-08T19:12Z.\n\nEstimated speed: ~828 km/s.\n\nEstimated opening half-angle: 38 deg.\n\nDirection (lon./lat.): -23/3 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T19:12:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Psyche (glancing blow), STEREO A, and Lucy (glancing blow).  The leading edge of the CME will reach STEREO A at 2024-05-11T06:45Z, and the flank of the CME may reach Psyche at 2024-05-15T20:00Z and Lucy at 2024-05-14T00:00Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-11T06:42Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 5-7 (minor to strong).\n   \n  \nLinks to the movies of the modeled event (includes CME: 2024-05-08T19:12:00-CME-001):\n\n(a) 2 AU outer boundary\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_2.0_ENLIL_CONE_STA_timeline.gif\n\n(b) 5.5 AU outer boundary\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_5.5_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_5.5_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_232700_5.5_ENLIL_CONE_Lucy_timeline.gif\n\n\n## Notes: \n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"SEP","messageID":"20240509-AL-004","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30611/1","messageIssueTime":"2024-05-09T14:00Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - SEP Prediction\n##\n## Message Issue Date: 2024-05-09T14:00:13Z\n## Message ID: 20240509-AL-004\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar energetic particle event forecasted at the orbit of SOHO starting at 2024-05-09T13:59Z.  The flux of one or more of the >15.8 MeV protons channels exceeds 10^(-1) pfu/MeV within next few hours.\n\nNASA spacecraft at the L1 and near-Earth orbits can be impacted.\"\n\n\nActivity ID: 2024-05-09T13:59:00-SEP-001.\n\n## Notes: \n\nThis SEP event (2024-05-09T13:59:00-SEP-001) is associated with an X2.2 flare from Active Region 13664 (S20W25) with ID 2024-05-09T08:45:00-FLR-001 which peaked at 2024-05-09T09:13Z (see notifications 20240509-AL-001 and 20240509-AL-002).\n\n\n\n"},{"messageType":"FLR","messageID":"20240509-AL-003","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30608/1","messageIssueTime":"2024-05-09T12:36Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - M9.8 Flare\n##\n## Message Issue Date: 2024-05-09T12:36:29Z\n## Message ID: 20240509-AL-003\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-08T22:05Z. \n\nFlare peak time: 2024-05-08T22:27Z.\n\nFlare intensity: M9.8 class.\n\nSource region: S22W22 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-08T22:05:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240509-AL-002","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30607/1","messageIssueTime":"2024-05-09T12:03Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X2.2 Flare\n##\n## Message Issue Date: 2024-05-09T12:03:16Z\n## Message ID: 20240509-AL-002\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-09T08:45Z. \n\nFlare peak time: 2024-05-09T09:13Z.\n\nFlare intensity: X2.2 class.\n\nSource region: S20W25 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-09T08:45:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240509-AL-001","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30606/1","messageIssueTime":"2024-05-09T09:00Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-09T09:00:46Z\n## Message ID: 20240509-AL-001\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-09T08:53Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-014","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30604/1","messageIssueTime":"2024-05-08T22:38Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-08T22:38:38Z\n## Message ID: 20240508-AL-014\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-08T21:28Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-013","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30602/1","messageIssueTime":"2024-05-08T22:35Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X1.0 Flare\n##\n## Message Issue Date: 2024-05-08T22:35:15Z\n## Message ID: 20240508-AL-013\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-08T21:00Z. \n\nFlare peak time: 2024-05-08T21:40Z.\n\nFlare intensity: X1.0 class.\n\nSource region: S20W17 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-08T21:00:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"Report","messageID":"20240508-7D-001","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30600/1","messageIssueTime":"2024-05-08T21:58Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information (CCMC DONKI)\n## Message Type: Weekly Space Weather Summary Report for May 01, 2024 - May 07, 2024\n##\n## Message Issue Date: 2024-05-08T21:58:42Z\n## Report Coverage Begin Date: 2024-05-01T00:00Z\n## Report Coverage End Date: 2024-05-07T23:59Z\n## Message ID: 20240508-7D-001\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSolar activity was at high levels during this reporting period with 4 X-class flares, 44 M-class flares, and 17 C-type CMEs (see details below).\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it was estimated that the following CMEs are predicted to impact missions near Earth:\n\nCME Starting time  | Predicted Impact (plus minus 7 hours)\n-----------------------------------------------------------------------------\n2024-05-03T02:48Z   NASA missions near Earth at 2024-05-06T06:00Z (glancing blow), Kp index 2-4 (below minor)\n                                       (see notification 20240503-AL-003)\n                                       The arrival of this CME may have been detected at L1 around 2024-05-05T11:30Z.\n2024-05-03T21:17Z   NASA missions near Earth at 2024-05-06T19:00Z (glancing blow), Kp index 3-5 (below minor to minor)\n                                       (see notification 20240504-AL-004)                                    \n                                       The arrival of this CME was not detected at L1.\n2024-05-03T21:28Z   NASA missions near Earth at 2024-05-06T19:00Z (glancing blow), Kp index 3-5 (below minor to minor)\n                                       (see notification 20240504-AL-004)                                    \n                                       The arrival of this CME was not detected at L1.\n\nIt was also estimated that the following CMEs are predicted to impact the listed locations:\n\nCME Starting time  | Predicted Impacts (plus minus 7 hours)\n-----------------------------------------------------------------------------\n2024-05-01T06:36Z    Parker Solar Probe at 2024-05-03T03:40Z, Lucy at 2024-05-07T03:00Z (glancing blow), Mars at 2024-05-05T16:00Z (glancing blow), OSIRIS-APEX at 2024-05-04T18:00Z (glancing blow), and STEREO A at 2024-05-04T20:00Z (glancing blow) (see notification 20240501-AL-002). \n2024-05-02T10:36Z    OSIRIS-APEX at 2024-05-06T02:13Z, Parker Solar Probe at 2024-05-04T16:26Z, Mars at 2024-05-07T01:00Z (glancing blow).\n2024-05-03T02:48Z    STEREO A at 2024-05-06T08:00Z (glancing blow) (see notification 20240503-AL-003). \n2024-05-03T21:17Z    STEREO A at 2024-05-06T18:00Z (glancing blow) (see notification 20240504-AL-004). \n2024-05-03T21:28Z    STEREO A at 2024-05-06T18:00Z (glancing blow) (see notification 20240504-AL-004).  \n\nNote: CME analyses from 2024-05-04 and 2024-05-05 were affected by a real-time coronagraph data outage.  Some CME parameters from these dates were not simulated due to simulation constraints.\n\nGeomagnetic activity was at strong levels with Kp index (a measure of geomagnetic activity, ranging 0-9) <=6.67 for the reporting period. The highest value of Kp=6.67 occurred during the synoptic periods of 2024-05-02T15:00Z-21:00Z (see notifications 20240502-AL-004, 20240502-AL-005, 20240502-AL-006). This strong enhancement of geomagnetic activity was associated with the interplanetary shock detected at L1 by ACE and DSCOVR around 2024-05-02T07:46Z (see notification 20240502-AL-001) which may be associated with a coronal hole high speed stream and potentially embedded glancing blow from a CME. The arrival of the coronal hole high speed stream was also detected by STEREO A on 2024-05-02.\n\nAdditionally, geomagnetic activity reached Kp=5 during the synoptic period of 2024-05-06T00:00Z-03:00Z. This minor enhancement of geomagnetic activity was associated with the interplanetary shock detected at L1 by ACE and DSCOVR around 2024-05-05T11:30Z which is associated with a possible glancing blow from the C-type CME first seen in SOHO LASCO imagery at 2024-05-03T02:48Z (see notification 20240503-AL-003) followed by a coronal hole high speed stream starting on 2024-05-06.\n\nThe > 2.0 MeV energetic electron flux detected at GOES remained below the threshold level of 1000 pfu for the entire reporting period. \n\nThe energetic proton flux of >10 MeV protons detected at GOES and the 13-100 MeV protons at STEREO A were all at background levels for the entire reporting period.\n\nSpace Weather Impact:\nSpace weather impacts on NASA spacecraft are expected to have been low to moderate this reporting period due to the geomagnetic activity described above.\n\n##Events:\nFlares (M-class and above)\nDate         Start     Stop      Peak      Class   Location         \n2024-05-01  14:17:00  14:37:00  14:32:00   M1.8   S07W71 ( 13654 ) \n2024-05-01  14:37:00  14:48:00  14:44:00   M1.9   S04W82 ( 13654 ) \n2024-05-01  22:26:00  22:37:00  22:31:00   M1.8   N25E22 ( 13663 ) \n2024-05-02  02:07:00  02:24:00  02:17:00   M1.0   N25E21 ( 13663 ) \n2024-05-02  20:52:00  21:01:00  20:57:00   M2.7   S21E58 ( 13664 ) \n2024-05-03  00:08:00  00:19:00  00:15:00   M2.7   S21E57 ( 13664 ) \n2024-05-03  02:11:00  02:27:00  02:22:00   X1.6   N26E05 ( 13663 ) \n2024-05-03  08:05:00  08:16:00  08:11:00   M4.4   N26E05 ( 13663 ) \n2024-05-03  22:25:00  23:11:00  22:47:00   M1.2   S08W100 ( 13654 )\n2024-05-03  23:11:00  23:20:00  23:16:00   M1.0   N25W04 ( 13663 ) \n2024-05-03  23:24:00  23:36:00  23:30:00   M2.4   N26W06 ( 13663 ) \n2024-05-04  00:26:00  00:44:00  00:36:00   M1.6   N26W05 ( 13663 ) \n2024-05-04  06:02:00  06:30:00  06:19:00   M9.1   N26W09 ( 13663 ) \n2024-05-04  07:04:00  07:11:00  07:07:00   M1.5   N27W08 ( 13663 ) \n2024-05-04  18:10:00  18:25:00  18:20:00   M1.3   N26W15 ( 13663 ) \n2024-05-04  22:23:00  22:54:00  22:37:00   M3.2   N26W15 ( 13663 ) \n2024-05-04  23:28:00  23:55:00  23:48:00   M9.0   N26W17 ( 13663 ) \n2024-05-05  01:15:00  01:43:00  01:27:00   M8.4   N26W20 ( 13663 ) \n2024-05-05  05:47:00  06:07:00  06:01:00   X1.3   N26W20 ( 13663 ) \n2024-05-05  08:07:00  08:24:00  08:19:00   M1.3   N26W22 ( 13663 ) \n2024-05-05  09:23:00  09:53:00  09:38:00   M2.3   S21E22 ( 13664 ) \n2024-05-05  09:53:00  10:19:00  10:00:00   M7.4   N26W22 ( 13663 ) \n2024-05-05  11:41:00  12:16:00  11:54:00   X1.2   N26W23 ( 13663 ) \n2024-05-05  14:33:00  14:56:00  14:47:00   M1.3   N26W24 ( 13663 ) \n2024-05-05  15:28:00  15:51:00  15:38:00   M2.2   N26W25 ( 13663 ) \n2024-05-05  16:55:00  17:06:00  17:01:00   M1.3   S18E24 ( 13664 ) \n2024-05-05  18:34:00  18:45:00  18:40:00   M1.0   S19E18 ( 13664 ) \n2024-05-05  19:44:00  20:06:00  19:52:00   M1.3   N26W28 ( 13663 ) \n2024-05-06  00:47:00  01:14:00  01:06:00   M1.6   N26W30 ( 13663 ) \n2024-05-06  05:09:00  05:38:00  05:28:00   M1.3   N26W37 ( 13663 ) \n2024-05-06  05:38:00  06:47:00  06:35:00   X4.5   N26W35 ( 13663 ) \n2024-05-06  09:49:00  10:04:00  09:59:00   M1.5   N26W38 ( 13663 ) \n2024-05-06  21:37:00  21:58:00  21:48:00   M1.2   N27W41 ( 13663 ) \n2024-05-06  21:58:00  23:07:00  22:27:00   M4.3   N27W42 ( 13663 ) \n2024-05-07  00:41:00  01:23:00  00:58:00   M2.6   N25W45 ( 13663 ) \n2024-05-07  05:58:00  06:27:00  06:16:00   M5.1   N27W47 ( 13663 ) \n2024-05-07  08:18:00  08:28:00  08:23:00   M1.3   N25W52 ( 13663 ) \n2024-05-07  08:28:00  08:33:00  08:31:00   M1.4   S18E05 ( 13668 ) \n2024-05-07  11:40:00  12:01:00  11:50:00   M2.4   S22W02 ( 13664 ) \n2024-05-07  12:43:00  12:59:00  12:54:00   M1.5   N25W54 ( 13663 ) \n2024-05-07  13:16:00  13:32:00  13:25:00   M1.0   N25W55 ( 13663 ) \n2024-05-07  13:32:00  13:39:00  13:35:00   M1.0   N25W55 ( 13663 ) \n2024-05-07  16:21:00  16:36:00  16:30:00   M8.2   N25W56 ( 13663 ) \n2024-05-07  19:58:00  20:34:00  20:22:00   M2.1   S21W12 ( 13664 ) \n2024-05-07  20:45:00  21:13:00  20:47:00   M1.2   S20W08 ( 13664 ) \n2024-05-07  21:13:00  21:42:00  21:26:00   M3.3   N26W57 ( 13663 ) \n2024-05-07  21:42:00  22:08:00  21:59:00   M3.3   N26W57 ( 13663 ) \n2024-05-07  22:55:00  23:35:00  23:31:00   M1.6   S11W09 ( 13664 ) \n\nCMEs (>500 km/s):\nEarth directed:\nStarting time        Speed (km/s)   Type   Direction (LON/LAT in HEEQ)   Half-Angle width (degrees)  Detecting spacecraft (real-time)  \n2024-05-03T02:48Z     ~972            C               -20/33                18                          SOHO, STEREO A                    \n2024-05-03T21:17Z     ~548            C               -32/14                26                          SOHO                              \n2024-05-03T21:28Z     ~509            C               -32/-13               18                          SOHO                              \n*2024-05-04T06:53Z     ~718            C                -9/37                17                          STEREO A, SOHO                    \n(* = updated parameters not simulated)\n\nNon-Earth directed (POS = Plane Of Sky):\nStarting time        Speed (km/s)   Type   Direction (LON/LAT in HEEQ)   Half-Angle width (degrees)  Detecting spacecraft (real-time)  \n2024-05-01T00:48Z     ~643            C         NONE(POS)/-53               21                          SOHO, STEREO A                    \n2024-05-01T06:36Z     ~794            C                65/-22               42                          SOHO, STEREO A                    \n2024-05-01T11:36Z     ~569            C               -25/59                20                          SOHO, STEREO A                    \n2024-05-01T12:36Z     ~524            C         NONE(POS)/-19               28                          SOHO, STEREO A                    \n2024-05-02T03:12Z     ~716            C               -21/52                14                          SOHO, STEREO A                    \n2024-05-03T09:24Z     ~672            C               -19/29                14                          SOHO, STEREO A                    \n2024-05-04T13:12Z     ~545            C         NONE(POS)/52                25                          SOHO, STEREO A                    \n*2024-05-05T02:09Z     ~516            C                -9/56                19                          STEREO A, SOHO                    \n*2024-05-05T13:24Z     ~533            C                -4/26                10                          SOHO                              \n*2024-05-05T15:48Z     ~642            C               -32/-20               32                          SOHO                              \n2024-05-05T17:00Z     ~756            C         NONE(POS)/24                35                          SOHO                              \n2024-05-06T07:38Z     ~510            C                10/40                17                          STEREO A                          \n2024-05-07T02:12Z     ~628            C               -75/-31               10                          SOHO, STEREO A                    \n(* = updated parameters not simulated)\n\n## Space Weather Outlook:\n## Outlook Coverage Begin Date: 2024-05-08T00:00Z \n## Outlook Coverage End Date:  2024-05-14T23:59Z\n\nSolar activity is expected to vary between moderate and high levels throughout the outlook period. There are currently six active regions on the Earth-facing disk. Active Regions 13663 (N25W68) and 13664 (S20W20) were responsible for 40 of the M-class flares and all of the X-class flares during the reporting period. Active Region 13664 is expected to continue moderate to high levels of flaring activity throughout the outlook period. Active Region 13663 is expected to rotate off of the Earth-facing disk on 2024-05-10, but is likely to still produce significant flares in the next couple of days. \n\nGeomagnetic activity is expected to vary between low to strong levels during the outlook period. Enhanced geomagnetic activity is expected starting on 2024-05-10 through 2024-05-11 due to the anticipated combined arrival of today's C-type halo CME first seen in SOHO LASCO imagery at 2024-05-08T05:36Z associated with the X1.0 class flare from Active Region 13664 and the C-type halo CME first seen in SOHO LASCO imagery at 2024-05-08T12:24Z associated with the M8.6 class flare from Active Region 13664. Further enhancement of geomagnetic activity is possible starting on 2024-05-12 from four coronal holes seen currently on the Earth-facing disk centered near (N07E27), (S35E10), (N25E05), and (N17W14). \n\n## Notes: \nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"CME","messageID":"20240508-AL-012","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30592/1","messageIssueTime":"2024-05-08T18:43Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Lucy, STEREO A, Parker Solar Probe, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-08T18:43:52Z\n## Message ID: 20240508-AL-012\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nC-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-08T05:36Z.\n\nEstimated speed: ~870 km/s.\n\nEstimated opening half-angle: 43 deg.\n\nDirection (lon./lat.): 9/-7 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T05:36:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Lucy, STEREO A, and Parker Solar Probe (glancing blow).  The leading edge will reach Lucy at 2024-05-12T08:48Z, STEREO A at 2024-05-10T07:28Z, and the leading edge or flank of the CME Parker Solar Probe at 2024-05-10T13:00Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-10T12:14Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 6-8 (moderate to severe).\n   \n  \nLinks to the movies of the modeled event (includes CME: 2024-05-08T05:36:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_ENLIL_CONE_STA_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_093000_2.0_ENLIL_CONE_Lucy_timeline.gif\n\n## Notes: \n\nThis CME event (2024-05-08T05:36:00-CME-001) is associated with M3.5 flare from AR 13664 (S21W10) with ID 2024-05-08T04:20:00-FLR-001 which peaked at 2024-05-08T04:30Z and X1.0 flare 13664 (S22W10) with ID 2024-05-08T04:37:00-FLR-001 which peaked at 2024-05-08T05:09Z (see notifications 20240508-AL-003, 20240508-AL-006).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-011","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30588/1","messageIssueTime":"2024-05-08T18:06Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - M7.9 Flare\n##\n## Message Issue Date: 2024-05-08T18:06:45Z\n## Message ID: 20240508-AL-011\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-08T17:32Z. \n\nFlare peak time: 2024-05-08T17:53Z.\n\nFlare intensity: M7.9 class.\n\nSource region: S17W13 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-08T17:32:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-010","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30587/1","messageIssueTime":"2024-05-08T17:54Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-08T17:54:34Z\n## Message ID: 20240508-AL-010\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-08T17:49Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"CME","messageID":"20240508-AL-009","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30575/1","messageIssueTime":"2024-05-08T16:50Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - CME (Lucy, STEREO A, Parker Solar Probe, Missions Near Earth)\n##\n## Message Issue Date: 2024-05-08T16:50:57Z\n## Message ID: 20240508-AL-009\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nC-type CME detected by STEREO A / SOHO. \n\nStart time of the event: 2024-05-08T12:24Z.\n\nEstimated speed: ~776 km/s.\n\nEstimated opening half-angle: 45 deg.\n\nDirection (lon./lat.): 3/-5 in Heliocentric Earth Equatorial coordinates.\n\nActivity ID: 2024-05-08T12:24:00-CME-001\n\nBased on preliminary analysis by the Moon to Mars Space Weather Analysis Office and heliospheric modeling carried out at NASA Community Coordinated Modeling Center, it is estimated that this CME may affect Lucy, STEREO A, and Parker Solar Probe (glancing blow).  The leading edge of the CME will reach Lucy at 2024-05-13T03:59Z, STEREO A at 2024-05-10T20:45Z, and flank of the CME will reach Parker Solar Probe at 2024-05-10T10:00Z (plus minus 7 hours). \n\nThe simulation also indicates that the CME may impact NASA missions near Earth. Simulations indicate that the leading edge of the CME will reach NASA missions near Earth at about 2024-05-11T01:39Z (plus minus 7 hours). The roughly estimated expected range of the maximum Kp index is 5-7 (minor to strong).\n   \n  \nLinks to the movies of the modeled event (includes CME: 2024-05-08T12:24:00-CME-001):\n\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_anim.tim-den.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_anim.tim-vel.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_anim.tim-den-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_anim.tim-vel-Stereo_A.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_ENLIL_CONE_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_ENLIL_CONE_PSP_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_ENLIL_CONE_STA_timeline.gif\nhttp://iswa.gsfc.nasa.gov/downloads/20240508_165800_2.0_ENLIL_CONE_Lucy_timeline.gif\n\n## Notes: \n\nThis CME event (2024-05-08T12:24:00-CME-001) is associated with M8.6 flare from AR 13664 (S20W11) with ID 2024-05-08T11:26:00-FLR-001 which peaked at 2024-05-08T12:04Z (see notifications 20240508-AL-005, 20240508-AL-007).\n\n\nSCORE CME typification system:\nS-type: CMEs with speeds less than 500 km/s\nC-type: Common 500-999 km/s\nO-type: Occasional 1000-1999 km/s\nR-type: Rare 2000-2999 km/s\nER-type: Extremely Rare >3000 km/s\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-008","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30563/1","messageIssueTime":"2024-05-08T13:45Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - M7.0 Flare\n##\n## Message Issue Date: 2024-05-08T13:45:34Z\n## Message ID: 20240508-AL-008\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-08T06:44Z. \n\nFlare peak time: 2024-05-08T06:53Z.\n\nFlare intensity: M7.0 class.\n\nSource region: S21W18 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-08T06:44:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-007","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30560/1","messageIssueTime":"2024-05-08T13:36Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - M8.5 Flare\n##\n## Message Issue Date: 2024-05-08T13:36:36Z\n## Message ID: 20240508-AL-007\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-08T11:26Z. \n\nFlare peak time: 2024-05-08T12:04Z.\n\nFlare intensity: M8.5 class.\n\nSource region: S20W11 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-08T11:26:00-FLR-001.\n\n## Notes: \n\nEruptive signatures, such as opening field lines and dimming, associated with this flare are observed in UV imagery. Analysis of associated coronal mass ejection observed in SOHO LASCO imagery is ongoing. \n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-006","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30558/1","messageIssueTime":"2024-05-08T13:10Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X1.0 Flare\n##\n## Message Issue Date: 2024-05-08T13:10:04Z\n## Message ID: 20240508-AL-006\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-08T04:37Z. \n\nFlare peak time: 2024-05-08T05:09Z.\n\nFlare intensity: X1.0 class.\n\nSource region: S22W10 (Active Region 13664) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-08T04:37:00-FLR-001.\n\n## Notes: \n\nThis X1.0 flare is associated with eruptive activity observed in SDO AIA imagery. Analysis of the associated coronal mass ejection observed in SOHO LASCO is ongoing. \n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-005","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30556/1","messageIssueTime":"2024-05-08T11:53Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-08T11:53:28Z\n## Message ID: 20240508-AL-005\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-08T11:47Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-004","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30554/1","messageIssueTime":"2024-05-08T06:55Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-08T06:55:24Z\n## Message ID: 20240508-AL-004\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-08T06:50Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-003","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30552/1","messageIssueTime":"2024-05-08T04:55Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-08T04:55:22Z\n## Message ID: 20240508-AL-003\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-08T04:49Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-002","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30550/1","messageIssueTime":"2024-05-08T01:55Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Space Weather Notification - X1.0 Flare\n##\n## Message Issue Date: 2024-05-08T01:55:42Z\n## Message ID: 20240508-AL-002\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n\nSignificant flare detected by GOES.\n\nFlare start time: 2024-05-08T01:33Z. \n\nFlare peak time: 2024-05-08T01:41Z.\n\nFlare intensity: X1.0 class.\n\nSource region: N25W60 (Active Region 13663) (based on SDO imagery).\n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\nActivity ID: 2024-05-08T01:33:00-FLR-001.\n\n## Notes: \n\n\n\n"},{"messageType":"FLR","messageID":"20240508-AL-001","messageURL":"https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/Alert/30549/1","messageIssueTime":"2024-05-08T01:43Z","messageBody":"## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )\n## Message Type: Auto-generated Space Weather Notification - Flare intensity has crossed the threshold of M5.0\n##\n## Message Issue Date: 2024-05-08T01:43:19Z\n## Message ID: 20240508-AL-001\n##\n## Disclaimer: NOAA's Space Weather Prediction Center is the United States Government official source for space weather forecasts. This \"Experimental Research Information\" consists of preliminary NASA research products and should be interpreted and used accordingly.\n\n\n## Summary:\n \n\nSignificant flare detected by GOES.  Flare intensity has crossed the threshold of M5.0.\n\nFlare M5.0 crossing time: 2024-05-08T01:39Z. \n\nIncreased energetic proton fluxes possible. Updates on this event will be provided when available.\n\n## Notes: \n\n\n\n"}]