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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-10T09:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-11-10T09:36:00-CME-001 (version 1)
Source Location: N25W16
Active Region Number: 14274
Note Keyword:
FOV: Front Bright front; may be evidence of pileup
HAL: Halo CME
OFL: Outflowing material at the back of the CME
SEP: Solar Energetic Particle event
Source Signature Keyword:
Morphology Keyword:
F: Flux Rope
FS: Flux Rope and Shock Candidate
Note: Halo CME seen in SOHO LASCO C2, SOHO LASCO C3, and GOES CCOR-1 and wide CME seen predominantly to the northeast in STEREO A COR2A in association with an eruptive X1.2-class solar flare from Active Region 14274 (N25W16). The solar flare is best seen in GOES SUVI 131 and a faint circular EUV wave is seen propagating shortly following the flare in GOES SUVI 195 and 284 angstrom imagers.
Version 1 submitted on 2025-11-10T12:31Z by Chris Stubenrauch
A Notification with ID
20251110-AL-006 was sent on 2025-11-10T12:36Z
A Notification with ID
20251110-AL-013 was sent on 2025-11-10T16:48Z
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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 |
SH
|
true |
SWPC_CAT |
11.0 |
8.0 |
1196.0 |
O |
56.0 |
2025-11-10T12:24Z |
Measurement of the shock front out to 13 solar radii. |
Not modeled
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2025-11-10T14:00Z |
Chris Stubenrauch on 2025-11-10T14:23Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
19.0 |
8.0 |
1298.0 |
O |
33.0 |
2025-11-10T11:42Z |
Updated bulk measurement out to 25 solar radii. |
1: Result 1 (2.0 AU)
Earth = 2025-11-12T03:27Z
BepiColombo = 2025-11-10T20:21Z
OSIRIS-APEX = 2025-11-11T18:30Z
Solar Orbiter = 2025-11-11T17:24Z
STEREO A = 2025-11-11T21:20Z
2: Result 2 (5.5 AU)
Earth = 2025-11-12T05:34Z
BepiColombo = 2025-11-10T20:20Z
OSIRIS-APEX = 2025-11-11T20:07Z
Solar Orbiter = 2025-11-11T17:41Z
STEREO A = 2025-11-11T21:14Z
3: Result 3 (2.0 AU)
Earth = 2025-11-11T16:53Z
BepiColombo = 2025-11-09T23:51Z
OSIRIS-APEX = 2025-11-11T06:54Z
Solar Orbiter = 2025-11-11T02:50Z
STEREO A = 2025-11-11T21:06Z
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2025-11-10T11:42Z |
Chris Stubenrauch on 2025-11-10T14:23Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
2.0 |
14.0 |
1208.0 |
O |
49.0 |
2025-11-10T12:07Z |
Preliminary measurement of the bulk with very few frames. |
Not modeled
|
2025-11-10T12:27Z |
Chris Stubenrauch on 2025-11-10T14:07Z |
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