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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-06-29T11:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-06-29T11:36:00-CME-001 (version 1)
Note Keyword:
OFL: Outflowing material at the back of the CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
Note: CME visible to the NW in SOHO LASCO C2/C3, STEREO A COR2 running difference imagery, and GOES CCOR-1. The CME is partially obscured by the pylon in SOHO LASCO C3. The potential source is a filament eruption on the NW limb as seen in GOES SUVI 304, with gradual filament liftoff starting around approximately 2025-06-29T10:45Z. Opening field lines also seen in SDO AIA 171/193. Eruption also visible in STEREO A EUVI 195/304. Additional outflowing material may follow this filament eruption.
Version 1 submitted on 2025-06-29T18:41Z 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
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
129.0 |
40.0 |
358.0 |
S |
18.0 |
2025-06-29T21:19Z |
Measurement based on best fit between SOHO LASCO C2, GOES CCOR-1, and STEREO A COR2 in SWPC_CAT. CME not measured in SOHO LASCO C3 because it is obscured by the pylon. |
1: Result 1 (2.0 AU)
Solar Orbiter = 2025-07-02T12:00Z
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Mary Aronne on 2025-06-29T18:42Z |
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