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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-06-16T08:23Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-06-16T08:23:00-CME-001 (version 2)
Note Keyword:
GAP: Data gap
Ha: Bright emission (likely H-alpha emission)
Source Signature Keyword:
FIL: Filament eruption
BR: Brightening
Morphology Keyword:
F: Flux Rope
Note: Bright CME visible to the NW in STEREO A COR2 and GOES CCOR-1 imagery. There is currently a data gap in SOHO LASCO C2/C3 imagery for this event. The source of the CME is a filament on/beyond the NW limb in SDO/AIA 304, GOES SUVI 304, and STEREO A EUVI 304 starting around 2025-06-16T04:15Z. Moving/opening field lines are visible beyond the NW limb in SDO/AIA 171 and 193, as well as in GOES SUVI 284.
Version 1 submitted on 2025-06-16T16:16Z by Carina Alden
Version 2 submitted on 2025-06-16T16:18Z 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 |
120.0 |
42.0 |
505.0 |
C |
36.0 |
2025-06-16T15:32Z |
Parameters based on best fit using STEREO A COR2 and GOES CCOR-1 imagery. There was no SOHO LASCO imagery available during this analysis. |
1: Result 1 (2.0 AU)
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Carina Alden on 2025-06-16T16:18Z |
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No Linked Activity Found. |
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