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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-24T20:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-05-24T20:48:00-CME-001 (version 2)
Note Keyword:
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
GAP: Data gap
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: Narrow CME to the west with the likely source an M-class flare and an associated minor eruption on/near the western limb seen starting around 2024-05-25T20:12Z in SDO AIA 304 imagery and as opening of field lines in AIA 193/171.
Submitted on 2025-02-07T18:04Z by Anna
Chulaki
A Notification with ID
20240525-AL-001 was sent on 2024-05-25T20:22Z
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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 |
90.0 |
4.0 |
854.0 |
C |
18.0 |
2024-05-25T01:00Z |
Analysis is based on the fit with two coronagraphs and confirmed by the location of the associated flare. |
1: Result 1 (2.0 AU)
Mars = 2024-05-29T05:56Z
Parker Solar Probe = 2024-05-26T17:21Z
OSIRIS-APEX = 2024-05-28T00:00Z
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Anna Chulaki on 2025-02-07T18:06Z |
CME Analysis
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M2M_CATALOG |
LE
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false |
Plane-of-sky |
NONE |
3.0 |
756.0 |
C |
21.0 |
2024-05-25T01:28Z |
Initial plane-of-sky analysis made with SOHO LASCO imagery, while STEREO imagery was not available. |
Not modeled
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Anna Chulaki on 2025-02-07T18:06Z |
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