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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-19T01:23Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-05-19T01:23:00-CME-001 (version 1)
Source Location: S40E10
Note Keyword:
DFL: Likely deflection of the event within the FOV
GAP: Data gap
Ha: Bright emission (likely H-alpha emission)
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
DFLR: Double ribbon flare
FIL: Filament eruption
OFL: Moving/Opening field lines
DIM: Dimming
Morphology Keyword:
F: Flux Rope
Note: Filament eruption seen to the SSE in all coronagraphs. Source is a long filament on-disk, spanning approximately S65E40->S35W20 (centered ~S40E10) at 2024-05-18T19:00Z, slowly rising and eventually lifting off from the disk. The filament extends a bit further SE, but that portion beyond ~S65E40 remains on the disk. Best observed as the filament erupting in SDO AIA 171/193/304, also as field line movement and dimming in SDO AIA 171/193, with a double ribbon flare in SDO AIA 304. A weak post-eruptive arcade is observed after the eruption as well.
Submitted on 2024-05-19T19:16Z by Tony
Iampietro
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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 |
-5.0 |
-47.0 |
426.0 |
S |
25.0 |
2024-05-19T07:51Z |
Triangulated measurement between SOHO LASCO and STEREO COR2A, using the rough center of the filament eruption ~S40E10 as an initial source, finding some southward deflection which may also be observed in AIA imagery. |
1: Result 1 (2.0 AU)
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Tony Iampietro on 2024-05-19T19:18Z |
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