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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-10-29T13:23Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C3
Activity ID: 2024-10-29T13:23:00-CME-001 (version 1)
Note Keyword:
GAP: Data gap
HAL: Halo CME
Source Signature Keyword:
PEA: Post eruption arcade
FIL: Filament eruption
BR: Brightening
Morphology Keyword:
Note: This event is visible for one frame in STEREO A COR2 imagery to the southwest, prior to a data gap from 2024-10-29T13:23Z to 23:23Z. In SOHO LASCO C3 this event is visible as a partial halo directed towards the southwest, but the CME is only observable for a few frames before it exits the field of view. The source is a large filament eruption spanning about S37W25 to S15W90, likely extending beyond the western limb, which begins to erupt around 2024-10-29T12:40Z as seen in SDO AIA 131, 171, 193, 304 imagery. Dimming is visible around the eruption site in SDO AIA 193 around 14:15Z, and post eruptive arcades begin to form around 17:15Z in SDO AIA 171 and 193 imagery.
Submitted on 2024-10-30T00:02Z by Mattie
Anastopulos
A Notification with ID
20241030-AL-001 was sent on 2024-10-30T01:16Z
A Notification with ID
20241030-AL-002 was sent on 2024-10-30T20:09Z
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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
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
46.0 |
-31.0 |
922.0 |
C |
47.0 |
2024-10-29T18:13Z |
BULK MEASUREMENT based on the approximate source location. This measurement relies on only a few frames of SOHO LASCO C3 imagery, for which the CME is near the end of the SOHO LASCO C3 field of view. Multiple measurements resulted in longitudes spanning 41 to 54 degrees and speeds ranging from 800 to 1054 km/s. This measurement is speculative due to the limited image availability at the time of this event. |
1: Result 1 (2.0 AU)
Earth = 2024-11-01T10:00Z
(PE: 14.5 h)
Mars = 2024-11-01T22:39Z
STEREO A = 2024-10-31T17:15Z
(PE: -6.8 h)
Solar Orbiter = 2024-10-31T18:00Z
2: Result 2 (5.5 AU)
Earth = 2024-11-01T10:00Z
(PE: 14.5 h)
Mars = 2024-11-01T22:19Z
STEREO A = 2024-10-31T16:58Z
(PE: -7.1 h)
Juno = 2024-11-11T06:00Z
Solar Orbiter = 2024-10-31T18:00Z
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Mattie Anastopulos on 2024-10-30T02:53Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
33.0 |
-21.0 |
1047.0 |
O |
52.0 |
2024-10-29T18:13Z |
SHOCK measurement based on the approximate source location tracking the faint, wider feature surrounding the bulk portion of this CME. This measurement is preliminary due to limited coronagraph imagery and the measured parameters may vary. |
1: Result 1 (2.0 AU)
Earth = 2024-10-31T19:19Z
(PE: -0.1 h)
Lucy = 2024-10-31T21:50Z
Mars = 2024-11-01T14:31Z
Solar Orbiter = 2024-10-31T03:59Z
STEREO A = 2024-10-31T10:50Z
(PE: -13.2 h)
2: Result 2 (5.5 AU)
Earth = 2024-10-31T19:10Z
(PE: -0.3 h)
Lucy = 2024-10-31T21:50Z
Mars = 2024-11-01T14:13Z
Solar Orbiter = 2024-10-31T03:53Z
STEREO A = 2024-10-31T10:36Z
(PE: -13.4 h)
Juno = 2024-11-11T00:00Z
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Mattie Anastopulos on 2024-10-30T02:53Z |
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