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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-05-01T09:38Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-05-01T09:38:00-CME-001 (version 2)
Source Location: S31W117
Active Region Number: 14065
Note Keyword:
Faint: Faint event; may affect type assignment
GAP: Data gap
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
Note: Narrow, fast CME to the SW in STEREO A COR2 and GOES CCOR-1. There is currently a data gap in SOHO LASCO C2 and C3 imagery. The source is seen as moving/opening field lines starting around 2025-05-01T08:39Z to the SW in SDO/AIA 193 and 171. An associated small filament eruption is also visible in SDO/AIA 304 and STEREO A EUVI 304 to the SW. This eruption is likely associated with old AR 14065 which rotated off the Earth-facing disk late on 2025-04-29. The estimated longitudes of the source are (~S31W110 to ~S31W125) based on calculation of average rotation and visible inspection of STEREO A EUV imagery. This active region is situated within a coronal hole which may attribute to deflection.

Submitted on 2025-05-06T16:15Z by Mary Aronne

No Notification has been sent for this activity yet.

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 117.0 -39.0 622.0 C 16.0 2025-05-01T15:15Z Parameters based on likely source location and best fit using STEREO A COR2 imagery. The longitude may vary by +/- 10 degrees due to limited stereoscopic viewpoints of source and CME. Not modeled Carina Alden on 2025-05-01T13:03Z



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