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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-12-13T14:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-12-13T14:48:00-CME-001 (version 1)
Note Keyword:
GAP: Data gap
OFL: Outflowing material at the back of the CME
Source Signature Keyword:
Morphology Keyword:
F: Flux Rope
Note: Wide CME seen predominantly to the south in SOHO LASCO imagery during a STEREO A data gap. May be potentially associated with an M1.0 flare from AR 3922 starting at 2024-12-13T14:15Z, but there is no clear eruption of material leading to a CME associated with it. There is some faint dimming seen in GOES SUVI 284 at 14:26Z, close in time to when this was in the coronagraphs. Initial analysis suggests this eruption originates from the far-side, but triangulation with STEREO A data is probably necessary to confirm front-sidedness.
Submitted on 2024-12-13T22:27Z by Chris
Stubenrauch
No Notification has been sent for this activity yet.
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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) |
Submitted By |
CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
180.0 |
-49.0 |
507.0 |
C |
42.0 |
2024-12-13T21:48Z |
Preliminary one spacecraft measurement assuming that the eruption originates from the far-side. |
Not modeled
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Chris Stubenrauch on 2024-12-13T22:28Z |
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