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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-27T20:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-05-27T20:12:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
Morphology Keyword:
Note: Faint narrow CME preceding the brighter and wider 2024-05-28T05:38Z CME likely from the same backsided source. No clear source have been found, although there is a slow movement of field lines in AIA 171 in the SW for a long time. There might be a super minor restructuring of magnetic field configuration likely far behind the SW limb seen in AIA 335 around 2024-05-27T20Z seen in AIA 335.

Submitted on 2024-05-28T17:53Z by Anna Chulaki

A Notification with ID 20240528-AL-001 was sent on 2024-05-28T18:43Z

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 127.0 -44.0 262.0 S 31.0 2024-05-28T09:36Z Very speculative analysis based on the fit in two coronagraphs. There is no clear source and the fit can have a range of longitudes, at least from 100 deg to 130 deg. 1: Result 1 (2.0 AU)
OSIRIS-APEX = 2024-05-31T08:00Z
Solar Orbiter = 2024-05-31T08:00Z
Anna Chulaki on 2025-02-07T00:59Z



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