Ειδοποιήσεις από το σύστημα έγκαιρης προειδοποίησης DONKI της NASA (διαστημικός καιρός, Ήλιος)
NASA DONKI Notifications
NASA DONKI Notifications
Message Type: CME
Message ID: 20250611-AL-002
Issue Time: 2025-06-11T02:33Z
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CMEs (BepiColombo, Mars)
##
## Message Issue Date: 2025-06-11T02:33:04Z
## Message ID: 20250611-AL-002
##
## 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.
## Summary:
Multiple CMEs have been detected as follows:
1: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-10T15:12Z.
Estimated speed: ~771 km/s.
Estimated opening half-angle: 22 deg.
Direction (lon./lat.): -80/31 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-10T15:12:00-CME-001
2: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-10T19:00Z.
Estimated speed: ~685 km/s.
Estimated opening half-angle: 29 deg.
Direction (lon./lat.): -85/25 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-10T19:00:00-CME-001
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 impact BepiColombo and Mars (minor impact). The leading edge of the CMEs will reach BepiColombo at 2025-06-11T16:51Z and Mars at 2025-06-15T00:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CMEs: 2025-06-10T15:12:00-CME-001, 2025-06-10T19:00:00-CME-001):
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CMEs update (Europa Clipper, BepiColombo, Mars)
##
## Message Issue Date: 2025-06-11T01:21:49Z
## Message ID: 20250611-AL-001
##
## 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.
## Summary:
Update on CMEs with IDs 2025-06-09T15:12:00-CME-001 and 2025-06-09T21:00:00-CME-001 (see previous notification 20250610-AL-001). 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 have little or no impact on Juno or Dawn.
Previous simulations also estimate that the CMEs may affect Europa Clipper (glancing blow), BepiColombo (glancing blow) and Mars (glancing blow). The flank of the CMEs will reach Europa Clipper at 2025-06-16T06:00Z, BepiColombo at 2025-06-10T09:00Z and Mars at 2025-06-14T21:00Z (plus minus 7 hours).
CME parameters are (C-type):
1: Start time of the event: 2025-06-09T15:12Z.
Estimated speed: ~948 km/s.
Estimated opening half-angle: 22 deg.
Direction (lon./lat.): -95/36 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-09T15:12:00-CME-001
2: Start time of the event: 2025-06-09T21:00Z.
Estimated speed: ~615 km/s.
Estimated opening half-angle: 16 deg.
Direction (lon./lat.): -90/27 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-09T21:00:00-CME-001
Links to the movies of the modeled event (includes CMEs: 2025-06-09T15:12:00-CME-001, 2025-06-09T21:00:00-CME-001):
(a) 2 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20250609_185700_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20250609_185700_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20250609_185700_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20250609_185700_2.0_ENLIL_CONE_Bepi_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20250609_185700_2.0_ENLIL_CONE_Mars_timeline.gif
(b) 5.5 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20250609_185800_5.5_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20250609_185800_5.5_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20250609_185800_5.5_ENLIL_CONE_EuropaClippr_timeline.gif
## Notes:
SCORE CME typification system:
S-type: CMEs with speeds less than 500 km/s
C-type: Common 500-999 km/s
O-type: Occasional 1000-1999 km/s
R-type: Rare 2000-2999 km/s
ER-type: Extremely Rare >3000 km/s
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CMEs (Lucy, Europa Clipper, BepiColombo, Mars)
##
## Message Issue Date: 2025-06-10T20:38:02Z
## Message ID: 20250610-AL-003
##
## 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.
## Summary:
Multiple CMEs have been detected as follows:
1: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-10T00:36Z.
Estimated speed: ~543 km/s.
Estimated opening half-angle: 20 deg.
Direction (lon./lat.): -90/34 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-10T00:36:00-CME-001
2: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-10T05:00Z.
Estimated speed: ~983 km/s.
Estimated opening half-angle: 12 deg.
Direction (lon./lat.): -80/27 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-10T05:00:00-CME-001
3: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-10T05:48Z.
Estimated speed: ~697 km/s.
Estimated opening half-angle: 24 deg.
Direction (lon./lat.): -89/26 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-10T05:48:00-CME-001
4: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-10T11:48Z.
Estimated speed: ~667 km/s.
Estimated opening half-angle: 18 deg.
Direction (lon./lat.): -80/20 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-10T11:48:00-CME-001
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 impact Lucy (glancing blow), Europa Clipper (glancing blow), BepiColombo (glancing blow), and Mars (glancing blow). The flank of the CMEs will reach Lucy at 2025-06-17T08:00Z, Europa Clipper at 2025-06-16T02:00Z, BepiColombo at 2025-06-11T01:00Z, and Mars at 2025-06-14T14:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CMEs: 2025-06-10T00:36:00-CME-001, 2025-06-10T05:00:00-CME-001, 2025-06-10T05:48:00-CME-001, 2025-06-10T11:48:00-CME-001):
(a) 2 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_2.0_ENLIL_CONE_Bepi_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_2.0_ENLIL_CONE_Mars_timeline.gif
(b) 5.5 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_5.5_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_5.5_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_5.5_ENLIL_CONE_Lucy_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_060200_5.5_ENLIL_CONE_EuropaClippr_timeline.gif
## Notes:
SCORE CME typification system:
S-type: CMEs with speeds less than 500 km/s
C-type: Common 500-999 km/s
O-type: Occasional 1000-1999 km/s
R-type: Rare 2000-2999 km/s
ER-type: Extremely Rare >3000 km/s
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (Europa Clipper, BepiColombo)
##
## Message Issue Date: 2025-06-10T18:48:50Z
## Message ID: 20250610-AL-002
##
## 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.
## Summary:
C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-10T06:36Z.
Estimated speed: ~611 km/s.
Estimated opening half-angle: 27 deg.
Direction (lon./lat.): -136/29 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-10T06:36:00-CME-001
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 Europa Clipper (glancing blow) and BepiColombo (glancing blow). The flank of the CME may reach Europa Clipper at 2025-06-16T04:00Z and BepiColombo at 2025-06-11T02:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CME: 2025-06-10T06:36:00-CME-001):
(a) 2 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20250610_122900_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_122900_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_122900_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_122900_2.0_ENLIL_CONE_Bepi_timeline.gif
(b) 5.5 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20250610_122900_5.5_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_122900_5.5_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20250610_122900_5.5_ENLIL_CONE_EuropaClippr_timeline.gif
## Notes:
SCORE CME typification system:
S-type: CMEs with speeds less than 500 km/s
C-type: Common 500-999 km/s
O-type: Occasional 1000-1999 km/s
R-type: Rare 2000-2999 km/s
ER-type: Extremely Rare >3000 km/s
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CMEs (BepiColombo, Mars)
##
## Message Issue Date: 2025-06-10T02:20:50Z
## Message ID: 20250610-AL-001
##
## 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.
## Summary:
Multiple CMEs have been detected as follows:
1: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-09T15:12Z.
Estimated speed: ~948 km/s.
Estimated opening half-angle: 22 deg.
Direction (lon./lat.): -95/36 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-09T15:12:00-CME-001
2: C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-09T21:00Z.
Estimated speed: ~615 km/s.
Estimated opening half-angle: 16 deg.
Direction (lon./lat.): -90/27 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-09T21:00:00-CME-001
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 impact BepiColombo (glancing blow) and Mars (glancing blow). The flank of the CMEs will reach BepiColombo at 2025-06-10T09:00Z and Mars at 2025-06-14T21:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CMEs: 2025-06-09T15:12:00-CME-001, 2025-06-09T21:00:00-CME-001):
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (BepiColombo)
##
## Message Issue Date: 2025-06-09T02:18:39Z
## Message ID: 20250609-AL-001
##
## 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.
## Summary:
C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2025-06-08T21:36Z.
Estimated speed: ~915 km/s.
Estimated opening half-angle: 16 deg.
Direction (lon./lat.): -122/31 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2025-06-08T21:36:00-CME-001
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 BepiColombo (glancing blow). The flank of the CME may reach BepiColombo at 2025-06-09T14:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CME: 2025-06-08T21:36:00-CME-001):
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - Interplanetary Shock
##
## Message Issue Date: 2025-06-08T18:52:53Z
## Message ID: 20250608-AL-002
##
## 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.
## Summary:
Significant interplanetary shock detected by DSCOVR at L1 at 2025-06-07T00:15Z.
The shock may be associated with the arrival of CME with ID 2025-06-03T07:48:00-CME-001. Magnetospheric compression and geomagnetic storm possible.
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - Continued Radiation Belt Enhancement
##
## Message Issue Date: 2025-06-08T16:34:44Z
## Message ID: 20250608-AL-001
##
## 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.
## Summary:
Significantly elevated energetic electron fluxes in the Earth's outer radiation belt. GOES "greater than 2.0 MeV" integral electron flux first crossed the threshold of 1000 pfu starting at 2025-06-02T15:05Z. The most recent crossing of the 1000 pfu threshold was at 2025-06-06T08:40Z and the fluxes are currently elevated but below the threshold.
The elevated energetic electron flux levels observed since 2025-06-02T15:05Z are likely caused by the CME with ID 2025-05-30T06:38:00-CME-001, CME with ID 2025-05-30T12:53:00-CME-001, CME with ID 2025-05-31T00:15:00-CME-001, and additional influence from the CME with ID 2025-05-31T14:23:00-CME-001 (see notifications 20250602-AL-004, 20250604-AL-001, and 20250606-AL-001).
NASA spacecraft at GEO, MEO and other orbits passing through or in the vicinity of the Earth's outer radiation belt can be impacted.
