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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-11-25T21:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-11-25T21:24:00-CME-001 (version 2)
Source Location: S12W25
Active Region Number: 13901
Note Keyword:
Faint: Faint event; may affect type assignment
GAP: Data gap
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
Note: This CME is visible to the south in SOHO LASCO C2, C3, and possibly to the SE in STEREO A COR2 imagery following a data gap. The CME is likely associated with the M1.9 flare from AR 13091 as seen from SDO/AIA 131 and associated dimming in SDO/AIA 193 starting around 20:33Z. The dimming and associated EUV wave is seen moving out in all directions, most notably seen to the north, east, and south of the source location. This CME event overlaps with CMEs visible to the southwest which began around 2024-11-25T18:00Z.
Submitted on 2025-02-04T21:23Z by Carina
Alden
A Notification with ID
20241126-AL-002 was sent on 2024-11-26T04:36Z
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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 |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-2.0 |
-23.0 |
935.0 |
C |
29.0 |
2024-11-26T00:31Z |
Parameters are based on best fit of feature in SOHO LASCO C3 imagery with guidance of directionality of features seen after a data gap in STEREO A COR2 imagery. Since the features aren't clear in STEREO A COR2 imagery it was not usable for this fit. Due to this, there is a higher degree of uncertainty with this CME analysis. |
1: Result 1 (2.0 AU)
Earth = 2024-11-28T06:48Z
(PE: -19.4 h)
Europa Clipper = 2024-11-28T12:39Z
Juice = 2024-11-27T11:30Z
Lucy = 2024-11-28T03:29Z
Solar Orbiter = 2024-11-28T04:16Z
STEREO A = 2024-11-28T03:24Z
(PE: -21.3 h)
Mars = 2024-11-29T16:00Z
2: Result 2 (5.5 AU)
Earth = 2024-11-28T06:18Z
(PE: -19.9 h)
Europa Clipper = 2024-11-28T12:08Z
Juice = 2024-11-27T11:11Z
Lucy = 2024-11-28T03:01Z
Solar Orbiter = 2024-11-28T03:55Z
STEREO A = 2024-11-28T03:07Z
(PE: -21.6 h)
Juno = 2024-12-10T02:00Z
Mars = 2024-11-29T16:00Z
3: Result 3 (2.0 AU)
Earth = 2024-11-28T06:25Z
(PE: -19.8 h)
Europa Clipper = 2024-11-28T12:54Z
Juice = 2024-11-27T11:34Z
Lucy = 2024-11-28T03:08Z
Solar Orbiter = 2024-11-28T04:26Z
STEREO A = 2024-11-28T03:13Z
(PE: -21.4 h)
4: Result 4 (5.5 AU)
Earth = 2024-11-28T06:05Z
(PE: -20.2 h)
Europa Clipper = 2024-11-28T12:29Z
Juice = 2024-11-27T11:13Z
Lucy = 2024-11-28T02:45Z
Solar Orbiter = 2024-11-28T04:09Z
STEREO A = 2024-11-28T02:56Z
(PE: -21.7 h)
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Carina Alden on 2024-11-26T03:54Z |
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