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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-03-25T00:45Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
SOHO: LASCO/C3
Activity ID: 2026-03-25T00:45:00-CME-001 (version 1)
Source Location: S14W52
Active Region Number: 14400
Note Keyword:
GAP: Data gap
Source Signature Keyword:
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
Note: CME visible to the southwest in GOES CCOR-1 and in limited available SOHO LASCO C3 imagery in real-time during a data downlink period. Not visible in STEREO A COR2 imagery due to a data gap starting at 2026-03-24T13:53Z. The source is a C2.9 flare and associated eruption from AR 14400 (approximately S14W52) starting at 2026-03-24T23:52Z as seen in GOES SUVI 195/284 with rapidly opening field lines and possible EUV wave.
Version 1 submitted on 2026-03-25T01:58Z by Mary Aronne
A Notification with ID
20260325-AL-001 was sent on 2026-03-25T13:27Z
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The List of CME Analysis already entered: |
| Event Type |
Catalog |
Measurement TypeCME measurement type: Leading Edge (LE), Shock Front (SH), Right Hand Boundary (RHB), Left Hand Boundary (LHB), Black/White Boundary (BW), Prominence Core (COR), Disconnection Front (DIS), Trailing Edge (TE). |
Prime?"primary flag" which is either True or False. If there are multiple CME analysis entries for a single CME, this flag would indicate which analysis is considered most accurate per measurement type. This is a helpful flag if you would like to download only one most accurate CME analysis per CME per Measurement Type |
Technique |
Long |
Lat |
Speed |
Type |
Half Width |
Time 21.5 |
Note |
WSA-ENLIL+Cone Result(s) |
Measured On |
Submitted By |
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CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
68.0 |
-19.0 |
1208.0 |
O |
23.0 |
2026-03-25T03:21Z |
Updated parameters based on SOHO LASCO C3 and GOES CCOR-1 imagery with matching to possible features in STEREO A COR2 following the data gap. Possible deflection within the FOV due to nearby CH. |
1: Result 1 (2.0 AU)
BepiColombo = 2026-03-25T17:26Z
STEREO A = 2026-03-26T17:30Z
Juice = 2026-03-28T12:00Z
OSIRIS-APEX = 2026-03-27T20:00Z
Parker Solar Probe = 2026-03-26T08:00Z
2: Result 2 (5.5 AU)
BepiColombo = 2026-03-25T17:15Z
STEREO A = 2026-03-26T17:21Z
Juice = 2026-03-28T12:00Z
Europa Clipper = 2026-03-29T12:00Z
OSIRIS-APEX = 2026-03-27T20:00Z
Parker Solar Probe = 2026-03-26T08:00Z
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Carina Alden on 2026-03-25T12:07Z |
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CME Analysis
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M2M_CATALOG |
LE
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false |
SWPC_CAT |
52.0 |
-17.0 |
1226.0 |
O |
20.0 |
2026-03-25T03:15Z |
Preliminary measurement based on the source location using 3 frames of available GOES CCOR-1 and SOHO LASCO C3 imagery. |
Not modeled
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2026-03-25T01:55Z |
Mary Aronne on 2026-03-25T01:59Z |
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