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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-02-05T02:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-02-05T02:12:00-CME-001 (version 1)
Note Keyword:
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
F: Flux Rope
Note: CME first visible to the SW in SOHO LASCO C2 starting at 2025-02-05T02:12Z. Also seen to the SW in SOHO LASCO C3 and to the S in STEREO A COR2. The source of this CME is a filament eruption from the SW quadrant of the Earth-facing disk easily seen across SDO EUV wavelengths. The filament is best seen beginning to lift off at approximately 2025-02-05T00:10Z in SDO AIA 304. The footpoints of the filament were located at approximately S35W27 and S30W65.

Submitted on 2025-02-05T14:17Z by Elizabeth Juelfs

A Notification with ID 20250205-AL-001 was sent on 2025-02-05T17:42Z

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 30.0 -42.0 708.0 C 30.0 2025-02-05T07:24Z Best fit measurement based on running difference imagery from SOHO LASCO C2/C3 and STEREO A COR2 and on the location of the erupting filament. 1: Result 1 (2.0 AU)
STEREO A = 2025-02-08T00:00Z
2: Result 2 (5.5 AU)
STEREO A = 2025-02-08T00:00Z
Elizabeth Juelfs on 2025-02-05T14:20Z



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