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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-02-12T22:18Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-02-12T22:18:00-CME-001 (version 3)
Note Keyword:
HAL: Halo CME
OFL: Outflowing material at the back of the CME
Source Signature Keyword:
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: The start of this CME is covered by gap in SOHO LASCO C3 and it is fully covered by gaps in SOHO LASCO C2 and STEREO A COR2. The source of this CME is an eruption behind the northeast limb starting at 2024-02-12T19:13Z and characterized by the opening of field lines, narrow ejecta (in SDO AIA 304) and the subsequent slowly appearing (peeking from behind limb) post-eruptive arcades seen in SDO AIA 171/193/304. This CME is associated with a long-duration occulted M2.6 class flare, likely associated with the post eruptive arcades peaking from behind the rim.
Submitted on 2025-02-07T23:55Z by Anna
Chulaki
A Notification with ID
20240213-AL-003 was sent on 2024-02-13T16:27Z
A Notification with ID
20240214-AL-002 was sent on 2024-02-14T13:42Z
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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 |
-116.0 |
14.0 |
999.0 |
C |
50.0 |
2024-02-13T00:28Z |
A very approximate analysis with one coronagraph (C3) in swpc_cat and with the source being behind the east limb. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2024-02-14T15:00Z
2: Result 2 (5.5 AU)
Juno = 2024-02-26T15:00Z
Parker Solar Probe = 2024-02-14T15:00Z
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Anna Chulaki on 2024-02-13T19:12Z |
CME Analysis
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M2M_CATALOG |
SH
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true |
SWPC_CAT |
-149.0 |
10.0 |
1121.0 |
O |
53.0 |
2024-02-13T00:05Z |
An uncertain analysis of halo-like fainter shock with one coronagraph in swpc_cat because of data gaps in other coronagraphs and with source being behind the east limb. |
Not modeled
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Anna Chulaki on 2024-02-13T19:11Z |
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Comments by users: |
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