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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-19T11:00Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
Activity ID: 2025-11-19T11:00:00-CME-001 (version 1)
Source Location: N15E90
Note Keyword:
GAP: Data gap
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
Note: CME visible to the NE in GOES CCOR-1. Not seen in SOHO LASCO C2/C3 in real-time due to a downlink gap, and not clearly visible in STEREO A COR2. The source is a C9.9 flare peaking at 2025-11-19T09:53Z from an unnumbered region on the NE limb as seen in GOES SUVI 131. Wide opening field lines can be best seen in GOES SUVI 171/195/284. 
Version 1 submitted on 2025-11-19T12:58Z by Mary Aronne
A Notification with ID 20251119-AL-003 was sent on 2025-11-19T16:32Z

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 19.0 582.0 C 17.0 2025-11-19T16:22Z Measurement based on approximate source location using GOES CCOR-1 imagery in SWPC_CAT. 1: Result 1 (2.0 AU)
Parker Solar Probe = 2025-11-21T01:00Z
Mary Aronne on 2025-11-19T13:01Z



All directly linked activities:
2025-11-19T09:29:00-FLR-001
FLR Type: C9.9


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