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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-23T23:30Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
Activity ID: 2025-11-23T23:30:00-CME-001 (version 1)
Source Location: S20W90
Note Keyword:
GAP: Data gap
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
F: Flux Rope
Note: Faint CME seen to the SW in GOES CCOR-1. Not yet seen in SOHO LASCO C2/C3 due to a scheduled data gap. Not yet seen in STEREO A COR2 due to data gap. This CME overlaps with a much brighter CME visible to the W in GOES CCOR-1. Source is a small filament eruption on the SW limb centered at S20W90, seen in GOES SUVI 304 as a rising loop of filamentary material and in GOES SUVI 284 as a rising loop with opening field lines, both seen starting at about 2025-11-23T22:34Z. This eruption is also seen in STEREO A EUVI 304 as brightening and in STEREO A EUVI 194 as dimming from the area.
Version 1 submitted on 2025-11-24T02:02Z by Hannah Hermann
	
A Notification with ID 20251124-AL-001 was sent on 2025-11-24T02:37Z

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 90.0 -23.0 865.0 C 21.0 2025-11-24T03:06Z Measurement using source location seen in available UV imagery and fit of the leading edge using several frames of GOES CCOR-1. This CME was not captured in real time by SOHO LASCO C2/C3 and STEREO A COR2 due to regularly scheduled data gaps for each instrument. 1: Result 1 (2.0 AU)
BepiColombo = 2025-11-24T19:00Z
STEREO A = 2025-11-26T22:00Z (PE: 3.2 h)
2: Result 2 (5.5 AU)
BepiColombo = 2025-11-24T19:00Z
STEREO A = 2025-11-26T22:00Z (PE: 3.2 h)
Hannah Hermann on 2025-11-24T02:05Z



All directly linked activities:
2025-11-26T18:48:00-IPS-001
Location: STEREO A


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