Message ID: 20260118-AL-001
Issue Time: 2026-01-18T00:25Z
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (Europa Clipper, Juice, STEREO A)
##
## Message Issue Date: 2026-01-18T00:25:45Z
## Message ID: 20260118-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: 2026-01-17T07:00Z.
Estimated speed: ~843 km/s.
Estimated opening half-angle: 26 deg.
Direction (lon./lat.): 82/-36 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2026-01-17T07:00:00-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 CME may impact Europa Clipper (minor impact), Juice (glancing blow), and STEREO A (glancing blow). The leading edge of the CME will reach Europa Clipper at 2026-01-24T12:00Z and its flanks will reach Juice at 2026-01-21T18:00Z and STEREO A at 2026-01-21T12:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CME: 2026-01-17T07:00:00-CME-001):
(a) 2 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_2.0_anim.tim-den-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_2.0_anim.tim-vel-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_2.0_ENLIL_CONE_STA_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_2.0_ENLIL_CONE_Juice_timeline.gif
(b) 5.5 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_5.5_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_5.5_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_120600_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
URL: View Details
GIFs:
Message ID: 20260117-AL-001
Issue Time: 2026-01-17T21:46Z
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (Lucy, Europa Clipper, Juice, STEREO A)
##
## Message Issue Date: 2026-01-17T21:46:57Z
## Message ID: 20260117-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:
O-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2026-01-17T03:00Z.
Estimated speed: ~1273 km/s.
Estimated opening half-angle: 14 deg.
Direction (lon./lat.): 90/3 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2026-01-17T03:00:00-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 CME may impact Lucy (minor impact), Europa Clipper (minor impact), Juice (glancing blow), and STEREO A (glancing blow). The leading edge of the CME will reach Lucy at 2026-01-30T04:00Z and Europa Clipper at 2026-01-23T12:00Z, and its flanks will reach Juice at 2026-01-21T04:00Z and STEREO A at 2026-01-21T04:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CME: 2026-01-17T03:00:00-CME-001):
(a) 2 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_2.0_anim.tim-den-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_2.0_anim.tim-vel-Stereo_A.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_2.0_ENLIL_CONE_STA_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_2.0_ENLIL_CONE_Juice_timeline.gif
(b) 5.5 AU outer boundary
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_5.5_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_5.5_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_5.5_ENLIL_CONE_Lucy_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260117_053800_5.5_ENLIL_CONE_EuropaClippr_timeline.gif
## Notes:
This CME event (2026-01-17T03:00:00-CME-001) is associated with C4.7 flare from Active Region 14336 (S09W88) with ID 2026-01-17T02:42:00-FLR-001 which peaked at 2026-01-17T02:46Z.
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
URL: View Details
GIFs:
Message ID: 20260116-AL-001
Issue Time: 2026-01-16T13:16Z
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: 2026-01-16T13:16:05Z
## Message ID: 20260116-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 remains elevated, recently crossing the threshold of 1000 pfu at 2026-01-16T12:05Z.
The elevated energetic electron flux levels observed since 2026-01-12T10:05Z (see notifications 20260112-AL-002 and 20260114-AL-001) are likely caused by the combined arrival of CME with ID 2026-01-08T05:53:00-CME-001 (see notifications 20260108-AL-001, 20260109-AL-002), CME with ID 2026-01-08T15:48:00-CME-001 (see notification 20260109-AL-003), CME with ID 2026-01-08T17:00:00-CME-001 (see notification 20260109-AL-001, 20260109-AL-003), and CME with ID 2026-01-08T17:12:00-CME-001 (see notification 20260109-AL-003).
NASA spacecraft at GEO, MEO and other orbits passing through or in the vicinity of the Earth's outer radiation belt can be impacted.
Activity ID: 2026-01-12T10:05:00-RBE-001.
## Notes:
The arrival of these CMEs is also associated with geomagnetic storm with ID 2026-01-10T18:00:00-GST-001 (see notifications 20260110-AL-004, 20260110-AL-005) and with magnetopause crossing with ID 2026-01-11T05:56:00-MPC-001 (see notification 20260111-AL-002).
URL: View Details
Message ID: 20260115-AL-003
Issue Time: 2026-01-15T20:52Z
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (Parker Solar Probe)
##
## Message Issue Date: 2026-01-15T20:52:53Z
## Message ID: 20260115-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:
C-type CME detected by STEREO A / GOES / SOHO.
Start time of the event: 2026-01-15T07:12Z.
Estimated speed: ~998 km/s.
Estimated opening half-angle: 35 deg.
Direction (lon./lat.): -120/39 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2026-01-15T07:12:00-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 Parker Solar Probe (cursory glancing blow). The flank of the CME may reach Parker Solar Probe at 2026-01-17T02:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CME: 2026-01-15T07:12:00-CME-001):
http://iswa.gsfc.nasa.gov/downloads/20260115_104000_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_104000_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_104000_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_104000_2.0_ENLIL_CONE_PSP_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
URL: View Details
GIFs:
Message ID: 20260115-AL-002
Issue Time: 2026-01-15T19:41Z
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (OSIRIS-APEX)
##
## Message Issue Date: 2026-01-15T19:41:03Z
## Message ID: 20260115-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 GOES / SOHO.
Start time of the event: 2026-01-15T00:36Z.
Estimated speed: ~561 km/s.
Estimated opening half-angle: 24 deg.
Direction (lon./lat.): 12/27 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2026-01-15T00:36:00-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 OSIRIS-APEX (glancing blow). The leading edge or flank of the CME will reach OSIRIS-APEX at 2026-01-18T00:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CME: 2026-01-15T00:36:00-CME-001):
http://iswa.gsfc.nasa.gov/downloads/20260115_053200_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_053200_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_053200_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_053200_2.0_ENLIL_CONE_Osiris_timeline.gif
## Notes:
This CME event (2026-01-15T00:36:00-CME-001) is associated with C3.8 flare from Active Region 14340 (N15E05) with ID 2026-01-14T23:33:00-FLR-001 which peaked at 2026-01-14T23:56Z.
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
URL: View Details
GIFs:
Message ID: 20260115-AL-001
Issue Time: 2026-01-15T14:27Z
Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (Mars, Psyche, Parker Solar Probe)
##
## Message Issue Date: 2026-01-15T14:27:35Z
## Message ID: 20260115-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: 2026-01-15T02:12Z.
Estimated speed: ~589 km/s.
Estimated opening half-angle: 43 deg.
Direction (lon./lat.): 170/38 in Heliocentric Earth Equatorial coordinates.
Activity ID: 2026-01-15T02:12:00-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 Mars (minor impact), Psyche (minor impact), and Parker Solar Probe (glancing blow). The leading edge or flank of the CME will reach Mars at 2026-01-19T12:00Z, Psyche at 2026-01-20T15:00Z, and Parker Solar Probe at 2026-01-17T06:00Z (plus minus 7 hours).
Links to the movies of the modeled event (includes CME: 2026-01-15T02:12:00-CME-001):
http://iswa.gsfc.nasa.gov/downloads/20260115_082300_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_082300_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_082300_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_082300_2.0_ENLIL_CONE_PSP_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_082300_2.0_ENLIL_CONE_Mars_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260115_082300_2.0_ENLIL_CONE_Psyche_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
URL: View Details
GIFs: