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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-31T18:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-07-31T18:36:00-CME-001 (version 1)
Source Location: S15W73
Active Region Number: 13768
Note Keyword:
GAP: Data gap
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 imagery, and is not seen in STEREO A COR2 due to a data gap. The source is likely an M5.3 flare and eruption from AR 3768 (S15W73) starting around 2024-07-31T18:05Z as seen in SDO AIA 131, 171, 193, 304 imagery. A wide opening of field lines is visible at this time in SDO AIA 171 and 193 imagery which appear to deflect north of the eruption site.
Submitted on 2024-08-01T12:57Z 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 |
73.0 |
2.0 |
1082.0 |
O |
45.0 |
2024-07-31T21:50Z |
Measured longitude based on the source location. Due to a data gap in STEREO A COR2 imagery, there is no stereoscopic viewpoint available to confirm the measurement. Additionally, the northern portion of this event is partially obscured by the pylon in SOHO LASCO C3. The measured parameters may vary slightly as a result. |
1: Result 1 (2.0 AU)
Mars = 2024-08-03T17:44Z
OSIRIS-APEX = 2024-08-02T09:58Z
Parker Solar Probe = 2024-08-03T04:00Z
STEREO A = 2024-08-03T08:00Z
(PE: -4.2 h)
2: Result 2 (5.5 AU)
Mars = 2024-08-03T17:00Z
OSIRIS-APEX = 2024-08-02T09:49Z
Juno = 2024-08-14T18:00Z
Parker Solar Probe = 2024-08-03T04:00Z
STEREO A = 2024-08-03T07:00Z
(PE: -5.2 h)
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: -4.2 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: -4.2 h)
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Mattie Anastopulos on 2024-08-01T17:42Z |
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CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
50.0 |
5.0 |
1109.0 |
O |
50.0 |
2024-07-31T21:43Z |
Measurement of the shock front using SOHO LASCO C3 imagery only. Because there is a data gap in STEREO A COR2 and this CME is partially obscured by the pylon in SOHO LASCO C3, the measured parameters may vary slightly. |
1: Result 1 (2.0 AU)
Earth = 2024-08-03T09:36Z
Mars = 2024-08-03T18:56Z
Parker Solar Probe = 2024-08-02T08:04Z
STEREO A = 2024-08-02T19:32Z
(PE: -16.6 h)
OSIRIS-APEX = 2024-08-02T14:00Z
2: Result 2 (5.5 AU)
Earth = 2024-08-03T09:20Z
Mars = 2024-08-03T18:11Z
Parker Solar Probe = 2024-08-02T07:45Z
STEREO A = 2024-08-02T19:21Z
(PE: -16.8 h)
Juno = 2024-08-14T12:00Z
OSIRIS-APEX = 2024-08-02T14:00Z
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Mattie Anastopulos on 2024-08-01T17:42Z |
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