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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-01-18T02:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-01-18T02:00:00-CME-001 (version 1)
Note Keyword:
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FIL: Filament eruption
DIM: Dimming
Morphology Keyword:
Note: This CME is visible to the N/NW in SOHO LASCO C2, C3, and to the N/NE in STEREO A COR2 following the front of the CME first seen in SOHO LASCO C2 at 2025-01-18T01:36Z. There are two potential sources for this CME. The first source of this CME could be associated with the same M1.7 flare from AR 3964 (N06W34) as the 18/01:36Z CME, however there is a simultaneous small filament eruption from an area to the SE of the main flaring AR location. This filament eruption (~S15W12) is the second potential source and is located above the large Earth-facing coronal hole which may have contributed to significant deflection of the CME.
Submitted on 2025-01-18T18:38Z by Carina
Alden
A Notification with ID
20250118-AL-002 was sent on 2025-01-18T21:34Z
A Notification with ID
20250118-AL-003 was sent on 2025-01-18T21:51Z
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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
|
true |
SWPC_CAT |
14.0 |
26.0 |
530.0 |
C |
24.0 |
2025-01-18T08:01Z |
Parameters based on best fit of CME using SOHO LASCO C3 and STEREO A COR2 imagery. Due to the overlapping nature of this CME and the CME first seen in SOHO LASCO C2 at 2025-01-18T01:36Z, there is a bit of uncertainty with the parameters. The separate front of this CME is more clearly seen in STEREO A COR2 imagery than it is in SOHO LASCO imagery, adding to the complexity of this analysis. |
1: Result 1 (2.0 AU)
Earth = 2025-01-20T20:00Z
Europa Clipper = 2025-01-22T02:00Z
Lucy = 2025-01-21T12:00Z
Mars = 2025-01-22T16:00Z
STEREO A = 2025-01-20T15:30Z
2: Result 2 (2.0 AU)
Earth = 2025-01-20T20:00Z
Europa Clipper = 2025-01-22T00:30Z
Juice = 2025-01-19T16:30Z
Lucy = 2025-01-21T11:00Z
Mars = 2025-01-22T15:30Z
STEREO A = 2025-01-20T09:00Z
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Carina Alden on 2025-01-18T18:42Z |
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