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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-09T18:23Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-05-09T18:23:00-CME-001 (version 1)
Source Location: S18W29
Active Region Number: 13664
Note Keyword:
FF: Event fails/disappears before exiting COR2
GAP: Data gap
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Partial halo CME associated with an X1.1 flare from AR 3664 (S18W29) with a full halo faint shock and slightly brighter fuzzy-fronted bulk. The start time is possibly earlier that 18:23Z as the start of this event is covered by a data gap in SOHO due to a maneuver. Coronal signatures include a large ejecta from AR 3664 seen starting north-westwards ~17:36ZZ in AIA 304, a significant-area dimming mostly extending northward and westward of the flare location and stretching as far as the two coronal holes north of the equator.
Submitted on 2024-05-09T22:26Z by Anna
Chulaki
A Notification with ID
20240509-AL-011 was sent on 2024-05-09T23:35Z
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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 |
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CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
30.0 |
-6.0 |
895.0 |
C |
44.0 |
2024-05-09T21:58Z |
Analysis of the slightly brighter, mostly western bulk front of this CME based on the location of the flare and dimming and on the good fit with two coronagraphs. |
1: Result 1 (2.0 AU)
Earth = 2024-05-11T07:55Z
(PE: -12.6 h)
Lucy = 2024-05-13T03:24Z
STEREO A = 2024-05-11T01:31Z
Parker Solar Probe = 2024-05-10T21:00Z
2: Result 2 (2.0 AU)
Earth = 2024-05-12T03:09Z
(PE: 6.7 h)
Lucy = 2024-05-13T23:29Z
STEREO A = 2024-05-11T21:13Z
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Anna Chulaki on 2024-05-09T22:32Z |
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CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
12.0 |
-5.0 |
1236.0 |
O |
45.0 |
2024-05-09T20:27Z |
Analysis of the fainter full halo shock front, made by fitting this front in two coronagraphs. |
1: Result 1 (2.0 AU)
Earth = 2024-05-10T19:02Z
(PE: -25.5 h)
Lucy = 2024-05-12T09:20Z
STEREO A = 2024-05-10T15:20Z
Parker Solar Probe = 2024-05-10T22:00Z
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Anna Chulaki on 2024-05-09T22:30Z |
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