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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-11-04T01:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-11-04T01:36:00-CME-001 (version 1)
Source Location: S04E42
Active Region Number: 13883
Note Keyword:
3P: 3-part structure CME
GAP: Data gap
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
F: Flux Rope
FS: Flux Rope and Shock Candidate
Note: Partial halo CME visible to the east in SOHO LASCO C2 and STEREO A COR2. The CME is visible in SOHO LASCO C3 after a data gap from 2024-11-04T02:18Z to 2024-11-04T05:43Z. The CME is associated with an M3.8 flare from AR 3883 (approximately S04E42) peaking at 2024-11-04T01:40Z. The eruption can be seen in all wavelengths of SDO AIA imagery, with brightening best seen in SDO AIA 131, dimming and EUV wave best seen in SDO AIA 193, and opening field lines best seen in SDO AIA 171. The eruption is also visible in STEREO A EUV imagery.
Submitted on 2024-11-04T13:13Z by Mary
Aronne
A Notification with ID
20241104-AL-001 was sent on 2024-11-04T14:03Z
A Notification with ID
20241104-AL-004 was sent on 2024-11-04T23:54Z
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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 |
-37.0 |
12.0 |
1067.0 |
O |
39.0 |
2024-11-04T04:54Z |
Measurement of the bulk of the CME based on the best fit between SOHO LASCO C2/C3 and STEREO A COR2 imagery in SWPC_CAT |
1: Result 1 (2.0 AU)
Earth = 2024-11-06T09:15Z
Lucy = 2024-11-05T18:12Z
Parker Solar Probe = 2024-11-05T17:36Z
Solar Orbiter = 2024-11-05T10:49Z
STEREO A = 2024-11-07T02:00Z
(PE: 9.7 h)
2: Result 2 (5.5 AU)
Earth = 2024-11-06T09:22Z
Lucy = 2024-11-05T18:08Z
Parker Solar Probe = 2024-11-05T18:08Z
Solar Orbiter = 2024-11-05T10:48Z
STEREO A = 2024-11-07T02:00Z
(PE: 9.7 h)
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Mary Aronne on 2024-11-04T13:15Z |
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