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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-14T01:25Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-11-14T01:25:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: CME seen to the SE in SOHO LASCO C2/C3 and GOES CCOR-1, and to the SSE in STEREO A COR2. Source is likely beyond the southeast limb of the Earth-facing disk. A rising loop of material may possibly be seen at 2025-11-13T23:35Z in STEREO A EUVI 195 from beyond the southeast limb. There are no source signatures discernable in GOES SUVI imagery. 
Version 1 submitted on 2025-11-14T19:09Z by Hannah Hermann
A Notification with ID 20251114-AL-011 was sent on 2025-11-14T20:14Z

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 -119.0 -37.0 1081.0 O 24.0 2025-11-14T04:13Z Measurement using best fit between several frames of SOHO LASCO C3 and STEREO A COR2 and the candidate source location seen in available UV imagery. 1: Result 1 (2.0 AU)
Parker Solar Probe = 2025-11-15T16:00Z
2: Result 2 (5.5 AU)
Parker Solar Probe = 2025-11-15T16:00Z
Hannah Hermann on 2025-11-14T19:11Z



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