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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-08-01T07:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-08-01T07:24:00-CME-001 (version 1)
Source Location: S15W80
Active Region Number: 13768
Note Keyword:
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
Morphology Keyword:
Note: This CME is visible as a partial halo to the west in SOHO LASCO C2/C3 and STEREO A COR2 coronagraph imagery. The source is an M8.2 flare and eruption from Active Region 13768 (S15W80) starting around 2024-08-01T07:00Z as seen in GOES SUVI 131, 171, 195, 284, 304 imagery. A wide opening of field lines is visible in GOES SUVI 171, 195, and 284 imagery at this time as well.
Submitted on 2024-08-01T13:26Z by Mattie
Anastopulos
A Notification with ID
20240801-AL-005 was sent on 2024-08-01T17:18Z
A Notification with ID
20240801-AL-006 was sent on 2024-08-01T17:29Z
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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 |
65.0 |
3.0 |
1092.0 |
O |
44.0 |
2024-08-01T10:49Z |
Measurement of the bulk portion based on the best fit between SOHO LASCO C3 and STEREO A COR2 coronagraphs. The measured longitude deflects about 15 degrees from the source location, and multiple measurements produced speeds ranging from 1092 km/s to 1120 km/s. |
1: Result 1 (2.0 AU)
Mars = 2024-08-04T07:37Z
STEREO A = 2024-08-03T17:35Z
(PE: -11.8 h)
OSIRIS-APEX = 2024-08-03T02:00Z
Parker Solar Probe = 2024-08-03T08:00Z
2: Result 2 (5.5 AU)
Mars = 2024-08-04T07:02Z
STEREO A = 2024-08-03T17:22Z
(PE: -12.1 h)
Juno = 2024-08-15T18:00Z
OSIRIS-APEX = 2024-08-03T02:00Z
Parker Solar Probe = 2024-08-03T08:00Z
3: Result 3 (2.0 AU)
Mars = 2024-08-03T17:44Z
OSIRIS-APEX = 2024-08-02T10:01Z
Parker Solar Probe = 2024-08-03T04:00Z
STEREO A = 2024-08-03T08:00Z
(PE: -21.4 h)
4: Result 4 (5.5 AU)
Mars = 2024-08-03T17:04Z
OSIRIS-APEX = 2024-08-02T09:49Z
Juno = 2024-08-14T00:00Z
Parker Solar Probe = 2024-08-03T04:00Z
STEREO A = 2024-08-03T08:00Z
(PE: -21.4 h)
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Mattie Anastopulos on 2024-08-01T17:40Z |
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CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
50.0 |
7.0 |
1100.0 |
O |
50.0 |
2024-08-01T10:49Z |
Measurement of the shock front based on the best fit between SOHO LASCO C3 and STEREO A COR2 imagery. |
1: Result 1 (2.0 AU)
Earth = 2024-08-03T09:36Z
(PE: -27.8 h)
Mars = 2024-08-03T18:56Z
Parker Solar Probe = 2024-08-02T08:04Z
STEREO A = 2024-08-02T19:32Z
(PE: -33.9 h)
OSIRIS-APEX = 2024-08-02T14:00Z
2: Result 2 (5.5 AU)
Earth = 2024-08-03T09:20Z
(PE: -28.0 h)
Mars = 2024-08-03T18:11Z
Parker Solar Probe = 2024-08-02T07:45Z
STEREO A = 2024-08-02T19:21Z
(PE: -34.1 h)
Juno = 2024-08-14T12:00Z
OSIRIS-APEX = 2024-08-02T14:00Z
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Mattie Anastopulos on 2024-08-01T17:40Z |
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