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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-01-21T10:53Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
Activity ID: 2025-01-21T10:53:00-CME-001 (version 3)
Source Location: S18E23
Active Region Number: 13967
Note Keyword:
DPL: CME exhibits dimpled front
FOV: Front Bright front; may be evidence of pileup
Ha: Bright emission (likely H-alpha emission)
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
DFLR: Double ribbon flare
FIL: Filament eruption
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright CME and faint shock to the SE in STEREO COR2A, not yet observed in SOHO LASCO C2/C3 due to a downlink gap except for a very few late SOHO C3 frames. The source is an M3.3 class flare from AR 3967 peaking at 2025-01-21T10:39Z. Starting around 2025-01-21T09:42Z, a wide area of the disk East and South of AR 13967 brightens up in SDO AIA 304/GOES SUVI 304 with observed filament ejecta fanning out to the SE. Field line movement and extensive dimming, with an EUV wave, over this area also observed in SDO AIA 171/193/211. Partially overlaps with far-sided CME: 2025-01-21T09:12Z.
Submitted on 2025-01-21T21:58Z by Chris
Stubenrauch
A Notification with ID
20250121-AL-001 was sent on 2025-01-21T21:55Z
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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 |
-23.0 |
-31.0 |
646.0 |
C |
37.0 |
2025-01-21T16:17Z |
Measurement using late SOHO C3 frames during a SOHO C2/C3 data gap occurring during early portions of the CME. |
1: Result 1 (2.0 AU)
Earth = 2025-01-24T06:54Z
Lucy = 2025-01-25T01:48Z
Solar Orbiter = 2025-01-24T03:08Z
Europa Clipper = 2025-01-25T18:00Z
Mars = 2025-01-26T08:00Z
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Chris Stubenrauch on 2025-01-21T21:08Z |
CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
-23.0 |
-31.0 |
585.0 |
C |
38.0 |
2025-01-21T16:54Z |
PRELIMINARY BULK single-spacecraft measurement with only available STEREO COR2A imagery as of this measurement, updated analysis will follow once SOHO imagery is available. Using the source longitude of E23 as a basis for this measurement with a potential range E10-E30 with the wide eruption signature observed in SDO AIA 304/GOES SUVI 304. |
1: Result 1 (2.0 AU)
Earth = 2025-01-24T12:55Z
Lucy = 2025-01-25T09:58Z
Solar Orbiter = 2025-01-24T05:31Z
Europa Clipper = 2025-01-26T02:00Z
Mars = 2025-01-26T18:00Z
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Tony Iampietro on 2025-01-21T14:22Z |
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