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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-09-27T03:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-09-27T03:00:00-CME-001 (version 3)
Source Location: N02E76
Active Region Number: 14232
Note Keyword:
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
Source Signature Keyword:
FLR: Flare
BR: Brightening
Morphology Keyword:
Note: Narrow jet-like CME to the ESE in all three coronagraphs (SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1). The source is likely a C3.6 flare from AR 14232 (N02E76) peaking at 2025-09-27T02:40Z best seen in GOES SUVI 131.
Version 1 submitted on 2025-09-27T17:48Z by Anna Chulaki
Version 2 submitted on 2025-10-06T15:59Z by Mary Aronne
Version 3 submitted on 2025-10-06T15:59Z by Mary Aronne
A Notification with ID
20250928-AL-001 was sent on 2025-09-28T00:40Z
A Notification with ID
20250928-AL-005 was sent on 2025-09-28T19:01Z
A Notification with ID
20250928-AL-006 was sent on 2025-09-28T19:30Z
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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
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-78.0 |
-7.0 |
1061.0 |
O |
10.0 |
2025-09-27T06:07Z |
Analysis based on the fit of this narrow jet with SOHO LASCO C2/C3 and STEREO A COR2 and in alignment with the possible source - a C class flare from AR14232. No good fit with this analysis for CCOR-1. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2025-09-27T22:00Z
2: Result 2 (2.0 AU)
Parker Solar Probe = 2025-09-27T22:33Z
Solar Orbiter = 2025-09-28T02:00Z
3: Result 3 (5.5 AU)
Parker Solar Probe = 2025-09-27T22:17Z
Psyche = 2025-10-01T19:00Z
Solar Orbiter = 2025-09-28T02:00Z
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Anna Chulaki on 2025-09-27T17:56Z |
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