DONKI: Menu Page
Go to:
|
DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-11-11T01:23Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-11-11T01:23:00-CME-001 (version 3)
Source Location: N20E25
Note Keyword:
DPL: CME exhibits dimpled front
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
Source Signature Keyword:
PEA: Post eruption arcade
FIL: Filament eruption
DIM: Dimming
Morphology Keyword:
LS: Loop and Shock Candidate
Note: A very faint but fast and relatively narrow CME with the fuzzy front that is only somewhat clearly seen in STEREO A COR2 running difference imagery. Its source is likely a relatively minor filament eruption seen starting around 2024-11-11T00:10Z, as seen in SDO AIA 304/193, GOES SUVI 304/195/284 and STEREO A EUVI 195. The filament is centered at ~N20E25 and stretches from N27E40 to N17E17. Coronal signatures of this CME include an ejecta seen erupting in SDO AIA 304 and a dimming and post-eruptive arcades seen in SDO AIA 193/195.
Version 1 submitted on 2024-11-11T14:03Z by Anna Chulaki
Version 2 submitted on 2024-11-11T14:25Z by Anna Chulaki
Version 3 submitted on 2025-02-08T00:45Z by Anna Chulaki
A Notification with ID
20241111-AL-001 was sent on 2024-11-11T16:58Z
|
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) |
Measured On |
Submitted By |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-25.0 |
19.0 |
984.0 |
C |
15.0 |
2024-11-11T04:24Z |
Approximate analysis based on the location of the source (the erupting filament) also confirmed by the fit of the front in two coronagraphs. |
1: Result 1 (2.0 AU)
Earth = 2024-11-14T00:00Z
(PE: -3.5 h)
Lucy = 2024-11-13T08:00Z
Solar Orbiter = 2024-11-13T02:00Z
2: Result 2 (5.5 AU)
Earth = 2024-11-14T00:00Z
(PE: -3.5 h)
Lucy = 2024-11-13T08:00Z
Solar Orbiter = 2024-11-13T02:00Z
|
2024-11-11T14:05Z |
Anna Chulaki on 2024-11-11T14:05Z |
|
All directly linked activities: |
|
|
|
| Comments by users: |
| 0 comment received. |
|
CCMC DONKI