NOAK Observatory (L02)

Alerts from NASA's DONKI Early Warning System (Space Weather, Sun)



NASA DONKI Notifications

NASA DONKI Notifications

Message Type: CME

Message ID: 20260124-AL-004

Issue Time: 2026-01-24T21:12Z

Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (BepiColombo, Mars, Parker Solar Probe, Psyche)
##
## Message Issue Date: 2026-01-24T21:12:29Z
## Message ID: 20260124-AL-004
##
## 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: 2026-01-24T10:53Z.

Estimated speed: ~664 km/s.

Estimated opening half-angle: 42 deg.

Direction (lon./lat.): -178/-46 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2026-01-24T10:53:00-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), Mars (glancing blow), Parker Solar Probe (glancing blow), and Psyche (glancing blow). The northern flank of the CME will reach BepiColombo at 2026-01-25T12:00Z, Mars at 2026-01-29T03:00Z, Parker Solar Probe at 2026-01-26T14:00Z, and Psyche at 2026-01-30T00:00Z (plus minus 7 hours).

Links to the movies of the modeled event (includes CME: 2026-01-24T10:53:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20260124_155400_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_155400_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_155400_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_155400_2.0_ENLIL_CONE_PSP_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_155400_2.0_ENLIL_CONE_Bepi_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_155400_2.0_ENLIL_CONE_Mars_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_155400_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:

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Message Type: CME

Message ID: 20260124-AL-003

Issue Time: 2026-01-24T20:24Z

Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (BepiColombo)
##
## Message Issue Date: 2026-01-24T20:24:06Z
## Message ID: 20260124-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: 2026-01-24T09:24Z.

Estimated speed: ~554 km/s.

Estimated opening half-angle: 33 deg.

Direction (lon./lat.): -90/0 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2026-01-24T09:24:00-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 will reach BepiColombo at 2026-01-25T18:00Z (plus minus 7 hours).


Links to the movies of the modeled event (includes CMEs: 2026-01-24T09:24:00-CME-001, 2026-01-24T09:48:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20260124_153900_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_153900_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_153900_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_153900_2.0_ENLIL_CONE_Bepi_timeline.gif


## Notes:
This CME was simulated with a C-type CME with Activity ID: 2026-01-24T09:48:00-CME-001.


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:

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Message Type: CME

Message ID: 20260124-AL-002

Issue Time: 2026-01-24T02:32Z

Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (BepiColombo, Parker Solar Probe)
##
## Message Issue Date: 2026-01-24T02:32:42Z
## Message ID: 20260124-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: 2026-01-23T22:28Z.

Estimated speed: ~987 km/s.

Estimated opening half-angle: 38 deg.

Direction (lon./lat.): -149/-54 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2026-01-23T22:28:00-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) and Parker Solar Probe (glancing blow). The flank of the CME may reach BepiColombo at 2026-01-24T20:00Z and Parker Solar Probe at 2026-01-25T22:00Z (plus minus 7 hours).

Links to the movies of the modeled event (includes CME: 2026-01-23T22:28:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20260124_021200_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_021200_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_021200_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_021200_2.0_ENLIL_CONE_PSP_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_021200_2.0_ENLIL_CONE_Bepi_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:

Notification GIF
Notification GIF
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Notification GIF

Message Type: CME

Message ID: 20260124-AL-001

Issue Time: 2026-01-24T01:31Z

Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (BepiColombo, Parker Solar Probe)
##
## Message Issue Date: 2026-01-24T01:31:43Z
## Message ID: 20260124-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 GOES / SOHO.

Start time of the event: 2026-01-23T17:12Z.

Estimated speed: ~520 km/s.

Estimated opening half-angle: 45 deg.

Direction (lon./lat.): -121/-25 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2026-01-23T17:12:00-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 BepiColombo and Parker Solar Probe (glancing blow). The leading edge of the CME will reach BepiColombo at 2026-01-24T22:19Z and the flank of the CME may reach Parker Solar Probe at 2026-01-26T02:00Z (plus minus 7 hours).

Links to the movies of the modeled event (includes CME: 2026-01-23T17:12:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20260124_013700_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_013700_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_013700_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_013700_2.0_ENLIL_CONE_PSP_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260124_013700_2.0_ENLIL_CONE_Bepi_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:

Notification GIF
Notification GIF
Notification GIF
Notification GIF
Notification GIF

Message Type: CME

Message ID: 20260123-AL-004

Issue Time: 2026-01-23T20:25Z

Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (BepiColombo, Parker Solar Probe, Psyche, Mars)
##
## Message Issue Date: 2026-01-23T20:25:13Z
## Message ID: 20260123-AL-004
##
## 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: 2026-01-23T15:12Z.

Estimated speed: ~687 km/s.

Estimated opening half-angle: 41 deg.

Direction (lon./lat.): -172/-36 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2026-01-23T15:12:00-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 BepiColombo, Parker Solar Probe, Psyche (minor impact), and Mars (glancing blow). The leading edge of the CME may reach BepiColombo at 2026-01-24T15:06Z, Parker Solar Probe at 2026-01-25T15:48Z, and Psyche at 2026-01-29T02:00Z. The flank of the CME may reach Mars at 2026-01-28T06:00Z (plus minus 7 hours).

Links to the movies of the modeled event (includes CME: 2026-01-23T15:12:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20260123_201600_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_201600_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_201600_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_201600_2.0_ENLIL_CONE_PSP_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_201600_2.0_ENLIL_CONE_Bepi_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_201600_2.0_ENLIL_CONE_Mars_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_201600_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:

Notification GIF
Notification GIF
Notification GIF
Notification GIF
Notification GIF
Notification GIF
Notification GIF

Message Type: CME

Message ID: 20260123-AL-003

Issue Time: 2026-01-23T17:44Z

Message Body: ## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Space Weather Notification - CME (Solar Orbiter)
##
## Message Issue Date: 2026-01-23T17:44:07Z
## Message ID: 20260123-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: 2026-01-23T03:00Z.

Estimated speed: ~659 km/s.

Estimated opening half-angle: 12 deg.

Direction (lon./lat.): 3/24 in Heliocentric Earth Equatorial coordinates.

Activity ID: 2026-01-23T03:00:00-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 Solar Orbiter (glancing blow). The flank of the CME may reach Solar Orbiter at 2026-01-24T22:00Z (plus minus 7 hours).

Links to the movies of the modeled event (includes CME: 2026-01-23T03:00:00-CME-001):

http://iswa.gsfc.nasa.gov/downloads/20260123_074300_2.0_anim.tim-den.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_074300_2.0_anim.tim-vel.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_074300_2.0_ENLIL_CONE_timeline.gif
http://iswa.gsfc.nasa.gov/downloads/20260123_074300_2.0_ENLIL_CONE_SolO_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:

Notification GIF
Notification GIF
Notification GIF
Notification GIF

Message Type: RBE

Message ID: 20260123-AL-002

Issue Time: 2026-01-23T13:36Z

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: 2026-01-23T13:36:44Z
## Message ID: 20260123-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:

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 2026-01-23T13:00Z.

The elevated energetic electron flux levels observed since 2026-01-21T09:30Z (see notification 20260121-AL-004) are caused by the arrival of CME with ID 2026-01-18T18:09:00-CME-001 (see notifications 20260118-AL-005, 20260119-AL-001, 20260119-AL-004, and 20260119-AL-005).

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: 2026-01-21T09:30:00-RBE-001.

## Notes:

The arrival of this CME was associated with a severe geomagnetic storm with ID 2026-01-19T18:00:00-GST-001 (see notifications 20260119-AL-007, 20260120-AL-001, 20260120-AL-002, and 20260121-AL-001). Simulations also indicated that the magnetopause separating magnetospheric and solar wind plasma was close to the geosynchronous orbit starting at 2026-01-19T22:49Z (see notification 20260119-AL-008).

URL: View Details


Message Type: SEP

Message ID: 20260123-AL-001

Issue Time: 2026-01-23T03:20Z

Message Body: *** This SEP event notification was triggered by a long data gap in STEREO A Beacon data from 2026-01-21T16:25Z to 2026-01-22T02:57Z. Once Beacon data returned, the 13-100 MeV proton flux was still above threshold which triggered an automatic notification with ID 20260122-AL-002 (see below).***

## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Auto-generated Space Weather Notification - SEP
##
## Message Issue Date: 2026-01-23T03:20:16Z
## Message ID: 20260123-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:

Solar energetic particle event detected by STEREO A. The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2026-01-23T03:05Z.

Activity ID: 2026-01-23T03:05:00-SEP-001.

## Notes:



URL: View Details


Message Type: SEP

Message ID: 20260122-AL-002

Issue Time: 2026-01-22T05:13Z

Message Body: *** From 2026-01-22T05:05Z to 2026-01-22T05:45Z, the GOES >10 MeV integral proton flux threshold exceeded 10 pfu as the original SEP event starting at 2026-01-18T22:55Z was declining below threshold. These points are not considered a separate SEP event as there was no additional flare or CME activity associated with this minor enhancement. The following automatic notification with ID 20260122-AL-002 was triggered (see below).***

## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Auto-generated Space Weather Notification - SEP
##
## Message Issue Date: 2026-01-22T05:13:54Z
## Message ID: 20260122-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:

Solar energetic particle event detected by GOES. The flux of > 10 MeV protons exceeds 10 pfu starting at 2026-01-22T05:05Z.

NASA spacecraft at MEO, GEO and other high-altitude orbits and high-inclination LEO can be impacted.

Activity ID: 2026-01-22T05:05:00-SEP-001.

## Notes:



URL: View Details


Message Type: SEP

Message ID: 20260122-AL-001

Issue Time: 2026-01-22T03:11Z

Message Body: *** This SEP event notification was triggered by a long data gap in STEREO A Beacon data from 2026-01-21T16:25Z to 2026-01-22T02:57Z. Once Beacon data returned, the 13-100 MeV proton flux was still above threshold which triggered an automatic notification with ID 20260122-AL-002 (see below).***

## Community Coordinated Modeling Center Database Of Notifications, Knowledge, Information ( CCMC DONKI )
## Message Type: Auto-generated Space Weather Notification - SEP
##
## Message Issue Date: 2026-01-22T03:11:54Z
## Message ID: 20260122-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:

Solar energetic particle event detected by STEREO A. The flux of 13-100 MeV protons exceeds 10^(-1) pfu/MeV starting at 2026-01-22T02:59Z.

Activity ID: 2026-01-22T02:59:00-SEP-001.

## Notes:



URL: View Details