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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-10-24T12:38Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
GOES: CCOR-1
Activity ID: 2025-10-24T12:38:00-CME-001 (version 1)
Note Keyword:
FF: Event fails/disappears before exiting COR2
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
Note: This CME is visible to the southeast in STEREO A COR2, SOHO LASCO C2, and GOES CCOR-1 for a few frames before becoming too diffuse to observe. This event is obscured by the pylon in SOHO LASCO C3 imagery. The source is likely related to a filament eruption spanning S15E50 to S10E38 which begins to lift off around 2025-10-24T12:00Z as seen in GOES SUVI 171/195/284/304 and STEREO A EUVI 304 imagery. The filament is located between two coronal holes and the associated CME likely exhibits deflection to the east as a result.
Version 1 submitted on 2025-10-24T19:30Z by Mattie Anastopulos
A Notification with ID
20251024-AL-003 was sent on 2025-10-24T20:01Z
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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 |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-59.0 |
-14.0 |
883.0 |
C |
12.0 |
2025-10-24T16:23Z |
Measurement based on the approximate source location and best fit between SOHO LASCO C2 and STEREO A COR2 imagery. The leading edge of this event becomes too diffuse to measure after a few frames. The measurement relies on early imagery as a result. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-10-25T08:37Z
Parker Solar Probe = 2025-10-26T04:00Z
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Mattie Anastopulos on 2025-10-24T19:33Z |
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All directly linked activities: |
| No Linked Activity Found. |
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