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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-29T05:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-11-29T05:48:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
Morphology Keyword:
Note: Peculiar-shaped pointy-nosed CME front seen to the NE in SOHO LASCO C2/C3 starting at 2025-11-29T05:48Z and to the NNE in STEREO A COR2. This front is accompanied by another, directly eastern, CME front and closely followed by several other CME fronts. (There are at least 4 distinct fronts best seen in STEREO A COR2 at the same timeframe). 
Version 1 submitted on 2025-11-29T20:29Z by Anna Chulaki
A Notification with ID 20251129-AL-004 was sent on 2025-11-29T23:28Z

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 -117.0 31.0 1402.0 O 27.0 2025-11-29T08:12Z Approximate analysis based on the fit of the front in three coronagraphs (SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1). The source is likely one of the lobes of what looks like a three-pronged prominence eruption from/behind the NE limb, seen starting at 2025-11-29T05:36Z in GOES SUVI 304. 1: Result 1 (2.0 AU)
Parker Solar Probe = 2025-11-30T02:10Z
Anna Chulaki on 2025-11-29T21:45Z



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