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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-04T00:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-11-04T00:24:00-CME-001 (version 4)
Source Location: N24E59
Active Region Number: 14274
Note Keyword:
3P: 3-part structure CME
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
DIM: Dimming
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME seen to the NE in SOHO LASCO C2 and GOES CCOR-1 and STEREO A COR2. Source is the C8.7 flare from AR 14274 (N24E59) peaking at 2025-11-04T00:08Z and an associated minor eruption with small ejecta seen in STEREO A EUV 304 on/behind the NE limb at 2025-11-04T00:45Z.
Version 1 submitted on 2025-11-04T02:25Z by Anna Chulaki
Version 2 submitted on 2025-11-04T18:31Z by Mary Aronne
Version 3 submitted on 2025-11-04T18:31Z by Mary Aronne
Version 4 submitted on 2025-11-08T16:00Z by Mary Aronne
A Notification with ID
20251104-AL-001 was sent on 2025-11-04T04:48Z
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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 |
-70.0 |
32.0 |
1055.0 |
O |
36.0 |
2025-11-04T04:17Z |
Final analysis with more imagery. It is based on the fit with all three coronagraphs (SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1) and on the source location of the M3.5 flare. This complex event associated with two flares is treated as a single CME. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-11-04T15:50Z
Parker Solar Probe = 2025-11-05T11:15Z
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Anna Chulaki on 2025-11-04T04:17Z |
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CME Analysis
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M2M_CATALOG |
SH
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true |
SWPC_CAT |
-63.0 |
26.0 |
945.0 |
C |
43.0 |
2025-11-04T04:26Z |
SHOCK measurement based on approximate source location and best fit in SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1. |
1: Result 1 (2.0 AU)
Earth = 2025-11-06T10:00Z
(PE: -7.8 h)
BepiColombo = 2025-11-04T14:31Z
Parker Solar Probe = 2025-11-05T12:53Z
OSIRIS-APEX = 2025-11-06T08:00Z
Solar Orbiter = 2025-11-06T06:00Z
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2025-11-04T12:36Z |
Melissa Kane on 2025-11-04T12:38Z |
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CME Analysis
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M2M_CATALOG |
LE
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false |
SWPC_CAT |
-44.0 |
31.0 |
700.0 |
C |
31.0 |
2025-11-04T05:28Z |
A very preliminary analysis with early imagery. This analysis is based on the location of the source (C8.7 flare) and on the fit with all three coronagraphs (SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1). |
Not modeled
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Anna Chulaki on 2025-11-04T04:15Z |
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