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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-11T10:23Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
GOES: CCOR-1
Activity ID: 2025-11-11T10:23:00-CME-001 (version 1)
Source Location: N27W27
Active Region Number: 14274
Note Keyword:
Ha: Bright emission (likely H-alpha emission)
HAL: Halo CME
OFL: Outflowing material at the back of the CME
SEP: Solar Energetic Particle event
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
LS: Loop and Shock Candidate
Note: Large halo CME first seen to the NE by STEREO A COR2 beginning at 2025-11-11T10:23Z, as well as to the NW by SOHO LASCO C2/C3 and GOES CCOR-1 in later frames. The source of this event is an X5.1 flare from Active Region 14274 (N27W27) which peaked at 2025-11-11T10:04Z as seen in GOES SUVI 131. Wide opening field lines and a large EUV wave and instance of dimming is visible in GOES SUVI 195 and 284 and STEREO A EUVI 195, along with post eruptive arcades visible in GOES SUVI 131 and 195.
Version 1 submitted on 2025-11-11T14:24Z by Melissa Kane
A Notification with ID
20251111-AL-010 was sent on 2025-11-11T14:57Z
A Notification with ID
20251111-AL-011 was sent on 2025-11-11T15:21Z
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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 |
22.0 |
24.0 |
1856.0 |
O |
45.0 |
2025-11-11T11:54Z |
BULK measurement based on approximate source location and best fit in SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1. |
1: Result 1 (2.0 AU)
Earth = 2025-11-12T20:05Z
BepiColombo = 2025-11-11T18:21Z
OSIRIS-APEX = 2025-11-12T13:16Z
Solar Orbiter = 2025-11-12T11:51Z
STEREO A = 2025-11-12T14:42Z
2: Result 2 (5.5 AU)
Earth = 2025-11-12T20:16Z
BepiColombo = 2025-11-11T18:15Z
OSIRIS-APEX = 2025-11-12T13:19Z
Solar Orbiter = 2025-11-12T11:54Z
STEREO A = 2025-11-12T14:39Z
Juno = 2025-11-21T12:00Z
3: Result 3 (2.0 AU)
Earth = 2025-11-12T06:10Z
BepiColombo = 2025-11-10T20:33Z
OSIRIS-APEX = 2025-11-11T20:30Z
Solar Orbiter = 2025-11-11T17:35Z
STEREO A = 2025-11-11T21:31Z
4: Result 4 (5.5 AU)
Earth = 2025-11-12T06:09Z
BepiColombo = 2025-11-10T20:22Z
OSIRIS-APEX = 2025-11-11T20:27Z
Solar Orbiter = 2025-11-11T17:31Z
STEREO A = 2025-11-11T21:19Z
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2025-11-11T14:19Z |
Melissa Kane on 2025-11-11T14:25Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
13.0 |
13.0 |
1715.0 |
O |
58.0 |
2025-11-11T12:08Z |
SHOCK measurement based on approximate source location and best fit in SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1. |
Not modeled
|
2025-11-11T15:06Z |
Melissa Kane on 2025-11-11T15:07Z |
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