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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-02-11T18:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-02-11T18:24:00-CME-001 (version 2)
Source Location: S10E90
Note Keyword:
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME seen to the E in SOHO LASCO C2/C3 and STEREO COR2A. The source is best observed in SDO AIA 304 as a filament eruption on the eastern limb around S10E90, beginning around 2025-02-11T17:48Z and erupting more explosively around 2025-02-11T18:04Z. Also observed as field line opening in SDO AIA 171/193, and a C7.2 flare peaking at 2025-02-11T18:25Z.
Submitted on 2025-02-12T03:04Z by Tony
Iampietro
A Notification with ID
20250212-AL-001 was sent on 2025-02-12T03:39Z
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The List of CME Analysis already entered: |
CME Analysis
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M2M_CATALOG |
SH
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true |
SWPC_CAT |
-90.0 |
-4.0 |
650.0 |
C |
37.0 |
2025-02-11T23:54Z |
SHOCK measurement of a faint feature traveling ahead and slightly faster than the brighter bulk feature. Triangulated measurement with SOHO LASCO C2/C3 and STEREO COR2A imagery, finding a good fit at E90, not as a plane-of-sky. |
1: Result 1 (2.0 AU)
OSIRIS-APEX = 2025-02-14T14:38Z
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Tony Iampietro on 2025-02-12T02:46Z |
CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-90.0 |
-3.0 |
565.0 |
C |
36.0 |
2025-02-12T00:34Z |
BULK measurement of the bright feature traveling slightly slower than the faint shock feature. Triangulated measurement with SOHO LASCO C2/C3 and STEREO COR2A imagery, finding a good fit at E90, not as a plane-of-sky. |
1: Result 1 (2.0 AU)
OSIRIS-APEX = 2025-02-14T18:11Z
2: Result 2 (5.5 AU)
OSIRIS-APEX = 2025-02-14T18:23Z
Juno = 2025-02-26T03:00Z
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Tony Iampietro on 2025-02-12T02:46Z |
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