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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-05-04T10:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-05-04T10:48:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
Note: Fast, diffuse CME to the SW in SOHO LASCO C2, C3, STEREO A COR2, and GOES CCOR-1. The source appears to be a filament eruption from beyond the SW limb of STEREO A EUVI 304 starting around 2025-05-04T10:15Z. Associated moving/opening field lines are visible in SDO/AIA 171 along the southern limb.
Submitted on 2025-05-04T18:32Z by Carina
Alden
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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
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
141.0 |
-57.0 |
648.0 |
C |
14.0 |
2025-05-04T16:19Z |
These parameters are based on best fit of feature using SOHO LASCO C3 and STEREO A COR2 imagery. The front is very diffuse and difficult to track which may have impacted the fit and these parameters. |
Not modeled
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Carina Alden on 2025-05-04T18:33Z |
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