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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-23T23:30Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
Activity ID: 2025-11-23T23:30:00-CME-001 (version 1)
Source Location: S20W90
Note Keyword:
GAP: Data gap
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
F: Flux Rope
Note: Faint CME seen to the SW in GOES CCOR-1. Not yet seen in SOHO LASCO C2/C3 due to a scheduled data gap. Not yet seen in STEREO A COR2 due to data gap. This CME overlaps with a much brighter CME visible to the W in GOES CCOR-1. Source is a small filament eruption on the SW limb centered at S20W90, seen in GOES SUVI 304 as a rising loop of filamentary material and in GOES SUVI 284 as a rising loop with opening field lines, both seen starting at about 2025-11-23T22:34Z. This eruption is also seen in STEREO A EUVI 304 as brightening and in STEREO A EUVI 194 as dimming from the area.
Version 1 submitted on 2025-11-24T02:02Z by Hannah Hermann
A Notification with ID
20251124-AL-001 was sent on 2025-11-24T02:37Z
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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
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
90.0 |
-23.0 |
865.0 |
C |
21.0 |
2025-11-24T03:06Z |
Measurement using source location seen in available UV imagery and fit of the leading edge using several frames of GOES CCOR-1. This CME was not captured in real time by SOHO LASCO C2/C3 and STEREO A COR2 due to regularly scheduled data gaps for each instrument. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-11-24T19:00Z
STEREO A = 2025-11-26T22:00Z
(PE: 3.2 h)
2: Result 2 (5.5 AU)
BepiColombo = 2025-11-24T19:00Z
STEREO A = 2025-11-26T22:00Z
(PE: 3.2 h)
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Hannah Hermann on 2025-11-24T02:05Z |
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