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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-31T08:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-07-31T08:00:00-CME-001 (version 1)
Source Location: S15W60
Active Region Number: 13768
Note Keyword:
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME seen to the west in SOHO LASCO C2/C3 and STEREO A COR2. Overlaps in the field of view with the narrower, more northern CME: 2024-07-31T07:12Z. The potential source may be a continuation of the eruption near AR 3768 characterized by opening field lines, and an EUV wave in GOES SUVI 195 and STEREO A EUV 195. This CME was determined to be a slower, separate feature from this CME.
Submitted on 2024-07-31T16:18Z by Mary
Aronne
No Notification has been sent for this activity yet.
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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 |
61.0 |
-1.0 |
434.0 |
S |
39.0 |
2024-07-31T15:27Z |
Due to poor difference imagery quality in SOHO LASCO C3 and STEREO A COR2, this is an approximate measurement with limited imagery. Measurements ranged from 430 km/s to approximately 600 km/s. |
1: Result 1 (2.0 AU)
Mars = 2024-08-03T15:00Z
OSIRIS-APEX = 2024-08-02T16:00Z
Parker Solar Probe = 2024-08-02T14:00Z
STEREO A = 2024-08-03T06:00Z
2: Result 2 (2.0 AU)
Mars = 2024-08-04T20:00Z
OSIRIS-APEX = 2024-08-02T16:00Z
Parker Solar Probe = 2024-08-03T02:00Z
STEREO A = 2024-08-03T20:00Z
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Mary Aronne on 2024-07-31T16:19Z |
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