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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-01-23T03:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2026-01-23T03:00:00-CME-001 (version 3)
Source Location: N30E01
Note Keyword:
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FIL: Filament eruption
DIM: Dimming
Morphology Keyword:
OS: Other and Shock Candidate
Note: Narrowish CME with messy front seen to the N in SOHO LASCO C2/C3 and GOES CCOR-1, following in the footsteps of CME: 2026-01-22T21:12Z. The CME is seen more clearly to NE in STEREO A COR2 after the nightly data gap ending at 2026-01-23T03:08Z. The front in STEREO is clear and bright in difference imagery, but there is also a fainter accompanying wider front as well in STEREO, possibly a very faint shock. The source could be a minor filament eruption seen after 2026-01-23T02Z centered around (N30E01), as seen in GOES SUVI 304.
Version 1 submitted on 2026-01-23T14:35Z by Anna Chulaki
Version 2 submitted on 2026-01-23T20:08Z by Anna Chulaki
Version 3 submitted on 2026-01-23T20:27Z by Anna Chulaki
A Notification with ID
20260123-AL-003 was sent on 2026-01-23T17:44Z
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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 |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
3.0 |
24.0 |
659.0 |
C |
12.0 |
2026-01-23T07:43Z |
Approximate analysis based on the fit of the front with two coronagraphs (SOHO LASCO and STEREO A COR2) and confirmed by the location of the likely source - a minor filament eruption centered (N30E01). |
1: Result 1 (2.0 AU)
Solar Orbiter = 2026-01-24T22:00Z
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Anna Chulaki on 2026-01-23T20:31Z |
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