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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-03-21T16:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2025-03-21T16:36:00-CME-001 (version 1)
Source Location: S17W33
Active Region Number: 14028
Note Keyword:
GAP: Data gap
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
DIM: Dimming
Morphology Keyword:
Note: CME visible to the SW in SOHO LASCO C2 and C3 imagery. No STEREO A COR2 imagery for this event due to a data gap. The source of this CME may be the M1.2 flare from AR14028 (S17W33) as seen in SDO/AIA 131 and 193. There is clear dimming and moving/opening field lines visible to the SW of the eruption suggesting deflection. This may be due to a coronal hole due north of the source location.
Submitted on 2025-03-22T00:46Z by Carina
Alden
No Notification has been sent for this activity yet.
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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 |
33.0 |
-20.0 |
391.0 |
S |
20.0 |
2025-03-22T01:17Z |
Parameters based on best fit using SOHO LASCO C3 imagery and the potential source location. Some uncertainty due to limited stereoscopic viewpoints. |
1: Result 1 (2.0 AU)
Solar Orbiter = 2025-03-23T03:59Z
STEREO A = 2025-03-24T15:00Z
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Carina Alden on 2025-03-22T00:51Z |
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