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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-02-15T13:25Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-02-15T13:25:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
FOV: Front Bright front; may be evidence of pileup
HAL: Halo CME
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright CME with a high southern latitude, seen to the west in STEREO A COR2 and almost exactly to the south in SOHO LASCO, indicating a backsided source. Coronal signatures include a huge prominence seen directly to the south in GOES SUVI 304 starting at 2025-02-12:56Z and originating behind the south limb, and also seen as an extensive movement of matter/field lines to the south and southeast in GOES SUVI 284, also likely happening behind the southern limb. Coronal signatures are almost not seen in SDO AIA, except for minimal movement of ejecta seen in AIA 304.

Submitted on 2025-02-15T18:34Z by Anna Chulaki

A Notification with ID 20250215-AL-004 was sent on 2025-02-15T21:45Z

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) Submitted By
CME Analysis M2M_CATALOG LE true SWPC_CAT 173.0 -43.0 820.0 C 37.0 2025-02-15T17:38Z Analysis based on the fit with two coronagraphs and corresponding well to the southern filament see in EUVI imagery. 1: Result 1 (2.0 AU)
BepiColombo = 2025-02-16T10:00Z
Parker Solar Probe = 2025-02-17T09:00Z
Anna Chulaki on 2025-02-15T18:35Z



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