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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-28T14:00Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-11-28T14:00:00-CME-001 (version 1)
Source Location: N30E90
Note Keyword:
GAP: Data gap
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
Note: This CME is visible to the E/NE in GOES CCOR-1, SOHO LASCO C2/C3 (following a data gap), and in STEREO A COR2 imagery to the north. The source appears to be a filament eruption visible beyond the E/NE limb in GOES SUVI 304 starting around 2025-11-28T13:04Z. Wide moving/opening field lines are also visible along the NE limb in GOES SUVI 284 starting around 2025-11-28T13:00Z.
Version 1 submitted on 2025-11-28T18:52Z by Carina Alden
	
A Notification with ID 20251128-AL-003 was sent on 2025-11-28T19:58Z

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 -127.0 28.0 525.0 C 43.0 2025-11-28T19:46Z Parameters based on best fit using GOES CCOR-1, STEREO A COR2, and SOHO LASCO C3 imagery. The CME feature in STEREO A COR2 imagery appears significantly more narrow than what is visible in SOHO LASCO C3 and GOES CCOR-1. This is possibly due to the different perspectives, but uncertainty of the parameters cannot be ignored. 1: Result 1 (2.0 AU)
Parker Solar Probe = 2025-11-30T01:04Z
Mars = 2025-12-02T08:00Z
2: Result 2 (2.0 AU)
Parker Solar Probe = 2025-11-29T12:00Z
Mars = 2025-12-02T08:00Z
Carina Alden on 2025-11-28T18:55Z



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