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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-10-25T07:53Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-10-25T07:53:00-CME-001 (version 3)
Source Location: S10E72
Active Region Number: 13873
Note Keyword:
GAP: Data gap
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
U: Unknown
Note: CME visible to the NE in STEREO A COR2 and SOHO LASCO C2/C3. The source is an M1.1 flare peaking at 2024-10-25T07:33Z from AR 3873 (approx. S10E72) as seen in SDO AIA 131. The eruption is best seen in GOES SUVI 304. The eruption is also visible in STEREO A EUV 195/304. In real-time, SOHO data was unavailable starting around 2024-10-24T12:48Z, but later backfilled.

Submitted on 2025-02-06T21:31Z by Mary Aronne

A Notification with ID 20241025-AL-002 was sent on 2024-10-25T13:09Z

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) Submitted By
CME Analysis M2M_CATALOG LE true SWPC_CAT -71.0 7.0 701.0 C 13.0 2024-10-25T12:35Z While SOHO white light imagery is not available for this event, running difference imagery is available for SOHO LASCO C2 and C3 in SWPC_CAT. 1: Result 1 (2.0 AU)
Parker Solar Probe = 2024-10-27T09:14Z
Mary Aronne on 2024-10-25T12:50Z



All directly linked activities:
2024-10-25T07:23:00-FLR-001
FLR Type: M1.1


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