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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-10-15T23:15Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-10-15T23:15:00-CME-001 (version 2)
Source Location: N25W55
Active Region Number: 14246
Note Keyword:
3P: 3-part structure CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME visible to the NW in GOES CCOR-1 and SOHO LASCO C2/C3. Visible to the north in STEREO A COR2. The source is an M2.7 flare peaking at 2025-10-15T22:28Z from Active Region 14246 (N25W55). An eruption with dimming, EUV wave, opening field lines, and post-eruption arcades is best seen in GOES SUVI 195 and from the point of view of STEREO A EUV 195.
Version 1 submitted on 2025-10-16T01:16Z by Mary Aronne
Version 2 submitted on 2025-10-16T01:18Z by Mary Aronne
A Notification with ID
20251016-AL-001 was sent on 2025-10-16T01:39Z
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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
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
48.0 |
37.0 |
750.0 |
C |
41.0 |
2025-10-16T03:29Z |
Updated leading edge measurement out to about 17 solar radii. |
Not modeled
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2025-10-16T11:58Z |
Chris Stubenrauch on 2025-10-16T11:59Z |
CME Analysis
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M2M_CATALOG |
LE
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false |
SWPC_CAT |
48.0 |
36.0 |
802.0 |
C |
33.0 |
2025-10-16T03:05Z |
Preliminary measurement based on primarily GOES CCOR-1 imagery in SWPC_CAT, with a few available frames of STEREO A COR2 and SOHO LASCO C2/C3 used as well. |
1: Result 1 (2.0 AU)
Solar Orbiter = 2025-10-17T12:00Z
STEREO A = 2025-10-18T06:00Z
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2025-10-16T01:11Z |
Mary Aronne on 2025-10-16T01:18Z |
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