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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-10-13T01:25Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-10-13T01:25:00-CME-001 (version 1)
Source Location: N24W12
Active Region Number: 14246
Note Keyword:
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
Source Signature Keyword:
FLR: Flare
BR: Brightening
Morphology Keyword:
Note: Faint CME seen to the west in SOHO LASCO C2/C3 and to the east in STEREO A COR2. Not clearly visible in GOES CCOR-1 imagery. The source is likely a C9.3 flare and eruption from AR 14246 (N24W12) best seen in GOES SUVI 131. The eruption is also visible with brightening in GOES SUVI 195 and STEREO A EUV 195.
Version 1 submitted on 2025-10-13T14:36Z by Mary Aronne
A Notification with ID
20251013-AL-003 was sent on 2025-10-13T15:57Z
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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
|
true |
SWPC_CAT |
17.0 |
6.0 |
589.0 |
C |
19.0 |
2025-10-13T06:45Z |
Measurement based on source location as well as the best fit between SOHO LASCO C2 and STEREO A COR2 imagery. The leading edge is not clearly measurable in SOHO LASCO C3 or GOES CCOR-1, and this measurement is based on limited imagery. Due to the faintness of the leading edge, this measurement is more approximate than usual. |
1: Result 1 (2.0 AU)
Earth = 2025-10-15T20:00Z
Solar Orbiter = 2025-10-14T13:43Z
OSIRIS-APEX = 2025-10-15T14:00Z
STEREO A = 2025-10-15T16:00Z
2: Result 2 (2.0 AU)
Earth = 2025-10-16T12:00Z
OSIRIS-APEX = 2025-10-16T08:34Z
Solar Orbiter = 2025-10-14T12:12Z
STEREO A = 2025-10-17T00:00Z
3: Result 3 (2.0 AU)
Earth = 2025-10-16T12:00Z
OSIRIS-APEX = 2025-10-16T09:03Z
Solar Orbiter = 2025-10-14T13:48Z
STEREO A = 2025-10-16T22:00Z
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2025-10-13T14:18Z |
Mary Aronne on 2025-10-13T14:38Z |
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