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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-03-13T06:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2026-03-13T06:24:00-CME-001 (version 1)
Source Location: N25E20
Note Keyword:
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
DIM: Dimming
Morphology Keyword:
Note: CME visible to the N/NE in SOHO LASCO C2/C3 and GOES CCOR-1. The CME overlaps in the field of view with CME: 2026-03-13T06:48Z in these coronagraphs. The CME is also visible to the NE in STEREO A COR2. There is at least one potential source eruption on the Earth-facing disk as seen in GOES SUVI 195 and 284 imagery, starting around 2026-03-13T05:44Z as dimming centered around N35W20. Additional dimming can be seen starting around the same time, centered around N25E20, and this is the more likely source candidate.
Version 1 submitted on 2026-03-13T15:11Z by Mary Aronne
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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) |
Measured On |
Submitted By |
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CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
-29.0 |
61.0 |
250.0 |
S |
24.0 |
2026-03-13T19:59Z |
Measurement based on the best fit between SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery in SWPC_CAT as well as the source location. |
Not modeled
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Mary Aronne on 2026-03-13T15:12Z |
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