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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-06-29T15:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-06-29T15:36:00-CME-001 (version 4)
Note Keyword:
3P: 3-part structure CME
HAL: Halo CME
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Wide bright CME seen to the west in SOHO LASCO C2/C3 and STEREO A COR2A, as well as in GOES CCOR-1 imagery. Its source is a prominent eruption of a long filament off the southwest limb seen in SDO AIA 304/193/171 imagery, as well as in EUVI A 195/304 imagery. The filament appears to be potentially wrapping around the limb in both SOHO and STEREO A instruments, so it is hard to estimate the center of this erupting filament. It looks like the filament breaks up in two parts, one seen almost off the west limb in EUVI A 304, and the other part likely having a lower longitude.
Version 1 submitted on 2025-06-29T23:56Z by Anna Chulaki
Version 2 submitted on 2025-06-30T10:52Z by Anna Chulaki
Version 3 submitted on 2025-06-30T10:57Z by Anna Chulaki
Version 4 submitted on 2025-06-30T17:34Z by Mary Aronne
A Notification with ID
20250630-AL-001 was sent on 2025-06-30T00:43Z
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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 |
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CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
141.0 |
-3.0 |
504.0 |
C |
35.0 |
2025-06-30T01:01Z |
Approximate analysis mostly based on the fit with three coronagraphs, but also taking into account that the filament is likely erupting from behind the west limb as seen in SDO AIA. |
1: Result 1 (2.0 AU)
Solar Orbiter = 2025-07-02T12:00Z
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Anna Chulaki on 2025-06-30T10:54Z |
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