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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-10-31T23:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
STEREO A: SECCHI/COR2
Activity ID: 2025-10-31T23:48:00-CME-001 (version 1)
Source Location: S08E40
Active Region Number: 14271
Note Keyword:
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
L: Loop
Note: Diffuse loop CME seen to the SE in SOHO LASCO C2 and GOES CCOR-1, and to the SE in STEREO A COR2. Source is an eruption from former AR 14271 (S08E40) seen as a bright ribbon of ejecta and opening field lines starting at 2025-10-31T23:02Z in GOES SUVI 304/284.
Version 1 submitted on 2025-11-01T17:56Z by Hannah Hermann
	
A Notification with ID 20251101-AL-005 was sent on 2025-11-01T19:16Z

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 -46.0 -18.0 567.0 C 32.0 2025-11-01T06:09Z Measurement using source location seen in available UV imagery and best fit between several frames of SOHO LASCO C2 and STEREO A COR2. Leading edge is too diffuse to reliably track in SOHO LASCO C3 and GOES CCOR-1. 1: Result 1 (2.0 AU)
Earth = 2025-11-04T04:00Z
BepiColombo = 2025-11-01T20:13Z
OSIRIS-APEX = 2025-11-03T16:00Z
Parker Solar Probe = 2025-11-03T04:00Z
Solar Orbiter = 2025-11-03T15:00Z
Hannah Hermann on 2025-11-01T17:57Z



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