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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-04-23T18:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-04-23T18:24:00-CME-001 (version 1)
Source Location: S19W60
Active Region Number: 13638
Note Keyword:
COL: Possible collision with previous CME
DPL: CME exhibits dimpled front
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME visible to the west/southwest in SOHO LASCO C2/C3 and STEREO A COR2. It may be associated with an eruption triggered by the M2.9 flare peaking at 2024-04-23T17:44Z from AR 3638, which also may have been associated with CME with ID: 2024-04-23T18:12:00-CME-001. The opening field lines appear to widen at 2024-04-23T17:51Z, which may be associated with this CME. It is analyzed as a separate feature from CME: 2024-04-23T18:12:00-CME-001 due to the difference in speed and apparent separate leading edge.
Submitted on 2024-04-24T16:13Z by Mary
Aronne
A Notification with ID
20240424-AL-003 was sent on 2024-04-24T17:45Z
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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, earlier measurements are marked as false when new or more accurate measurements are made. This is a helpful flag if you would like to download only one most accurate CME analysis per CME |
Technique |
Long |
Lat |
Speed |
Type |
Half Width |
Time 21.5 |
Note |
WSA-ENLIL+Cone Result(s) |
Submitted By |
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CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
60.0 |
-34.0 |
444.0 |
S |
47.0 |
2024-04-24T02:43Z |
Limited imagery available for this measurement due to the faintness of the leading edge in difference imagery. |
1: Result 1 (2.0 AU)
Lucy = 2024-04-30T20:00Z
Mars = 2024-04-28T18:00Z
OSIRIS-APEX = 2024-04-27T12:00Z
Parker Solar Probe = 2024-04-26T00:00Z
STEREO A = 2024-04-27T10:00Z
2: Result 2 (5.5 AU)
Lucy = 2024-04-30T20:00Z
Mars = 2024-04-28T18:00Z
OSIRIS-APEX = 2024-04-27T12:00Z
Parker Solar Probe = 2024-04-26T00:00Z
STEREO A = 2024-04-27T10:00Z
3: Result 3 (2.0 AU)
Earth = 2024-04-26T22:00Z
Lucy = 2024-04-30T20:00Z
OSIRIS-APEX = 2024-04-27T12:00Z
Parker Solar Probe = 2024-04-26T00:00Z
Psyche = 2024-04-30T00:00Z
STEREO A = 2024-04-26T22:00Z
4: Result 4 (5.5 AU)
Earth = 2024-04-26T22:00Z
Lucy = 2024-04-30T20:00Z
OSIRIS-APEX = 2024-04-27T12:00Z
Parker Solar Probe = 2024-04-26T00:00Z
Psyche = 2024-04-30T00:00Z
STEREO A = 2024-04-26T22:00Z
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Mary Aronne on 2024-04-24T16:14Z |
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