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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-24T08:23Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
Activity ID: 2024-07-24T08:23:00-CME-001 (version 1)
Source Location: S08W60
Active Region Number: 13751
Note Keyword:
FF: Event fails/disappears before exiting COR2
GAP: Data gap
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
BR: Brightening
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME visible to the west in STEREO A COR2. Not visible in SOHO LASCO C2/C3 in real time due to a data gap. The source is likely an M3.6 flare peaking at 2024-07-24T07:42Z from AR 3751 (approx. S08W60). There is a gap in SDO AIA imagery from ~2024-07-24T06:48Z to 07:45Z, but the eruption is visible in STEREO A EUV 195 and GOES SUVI imagery. The flare is best seen in GOES SUVI 131, EUV wave and opening field lines are visible in STEREO A EUV 195 and GOES SUVI 195/171 starting around 2024-07-24T07:40Z.
Submitted on 2024-07-24T12:14Z by Mary
Aronne
A Notification with ID
20240724-AL-002 was sent on 2024-07-24T12:56Z
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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
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true |
SWPC_CAT |
60.0 |
8.0 |
552.0 |
C |
28.0 |
2024-07-24T14:17Z |
Measurement using STEREO A COR2 imagery only due to lack of SOHO imagery. Longitude based on approximate source location. |
1: Result 1 (2.0 AU)
Mars = 2024-07-28T16:00Z
OSIRIS-APEX = 2024-07-26T17:00Z
Parker Solar Probe = 2024-07-26T16:00Z
STEREO A = 2024-07-27T18:00Z
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Mary Aronne on 2024-07-24T12:52Z |
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CME Analysis
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M2M_CATALOG |
SH
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true |
SWPC_CAT |
60.0 |
12.0 |
701.0 |
C |
30.0 |
2024-07-24T12:42Z |
Measurement of the wider, faint, faster shock feature ahead of the leading edge of the CME. This measurement using STEREO A COR2 imagery only due to lack of available SOHO imagery, and the longitude is based on the approximate source location. |
1: Result 1 (2.0 AU)
Mars = 2024-07-28T08:03Z
OSIRIS-APEX = 2024-07-26T13:00Z
Parker Solar Probe = 2024-07-26T12:00Z
STEREO A = 2024-07-27T12:00Z
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Mary Aronne on 2024-07-24T12:52Z |
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