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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-12T23:06Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-07-12T23:06:00-CME-001 (version 1)
Note Keyword:
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
GAP: Data gap
HAL: Halo CME
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: A very faint but fast partial halo CME covered by a data gap in SOHO LASCO C2 and STEREO A COR2 and first seen in C3. The source (initially very hard to identify) was found in GOES SUVI 304 as a long but faint filament erupting (likely) behind the ENE limb starting at 2024-07-12T22:50Z.

Submitted on 2024-07-13T16:22Z by Anna Chulaki

A Notification with ID 20240717-AL-003 was sent on 2024-07-17T16:50Z

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 M2M_CATALOG LE true SWPC_CAT -116.0 1.0 1190.0 O 24.0 2024-07-13T01:26Z Approximate analysis of the brighter narrower bulk front of this CME based on the best fit in two coronagraphs, somewhat confirmed by the potential source - a behind the ENE limb filament. 1: Result 1 (2.0 AU)
2: Result 2 (5.5 AU)
Psyche = 2024-07-19T10:00Z
Anna Chulaki on 2024-07-13T16:35Z
CME Analysis M2M_CATALOG SH true SWPC_CAT -136.0 3.0 1218.0 O 43.0 2024-07-13T01:27Z Approximate analysis of the fainter and wider likely shock front of this CME based on the fit in two coronagraphs. Not modeled Anna Chulaki on 2024-07-13T16:35Z



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