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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-02-24T20:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2023-02-24T20:36:00-CME-001 (version 4)
Source Location: N29W24
Active Region Number: 13229
Note Keyword:
3P: 3-part structure CME
FOV: Front Bright front; may be evidence of pileup
Ha: Bright emission (likely H-alpha emission)
PRM: Prominence material (filamentary structures)
SEP: Solar Energetic Particle event
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Partial halo CME seen mostly to the NW in SOHO LASCO and STEREO A COR2A coronagraphs. The CME is associated with an M3.7-class flare and subsequent eruption from AR3229. The flare induces a large nearby filament channel to break and lift off seen best in SDO/GOES 304, but also in SDO 193 and GOES-16 195. The flare and CME are also associated with a small enhancement in 10 MeV protons observed at GOES.
Submitted on 2023-03-01T19:56Z by Mary
Aronne
A Notification with ID
20230224-AL-002 was sent on 2023-02-24T23:50Z
A Notification with ID
20230225-AL-008 was sent on 2023-02-25T21:52Z
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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 |
19.0 |
29.0 |
1276.0 |
O |
41.0 |
2023-02-24T23:14Z |
Remeasured using SOHO LASCO C3 imagery. This measurement does not include the shock halo. |
1: Result 1 (2.0 AU)
Earth = 2023-02-26T15:20Z
(PE: -3.4 h)
OSIRIS-REx = 2023-03-01T01:32Z
Solar Orbiter = 2023-02-27T06:00Z
STEREO A = 2023-02-26T20:00Z
(PE: 5.5 h)
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Chris Stubenrauch on 2023-02-26T15:35Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
20.0 |
24.0 |
1441.0 |
O |
39.0 |
2023-02-24T23:01Z |
This is a very preliminary measurement with only 4 frames in STEREO A using SWPC_Cat. The CME leading edge is better visible in the last few frames so the shock is not accounted here for. The particles are getting elevated in all instruments, SOHO, STA and GOES. There is a big EUV wave seen towards Earth in SDO images (171/193). The CME needs to be remeasured when SOHO C3 images come in. |
1: Result 1 (2.0 AU)
Earth = 2023-02-26T13:46Z
(PE: -5.0 h)
STEREO A = 2023-02-26T17:38Z
(PE: 3.1 h)
OSIRIS-REx = 2023-02-28T16:00Z
Solar Orbiter = 2023-02-27T03:00Z
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Yaireska Collado on 2023-02-24T22:49Z |
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CME Analysis
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M2M_CATALOG |
LE
|
false |
SWPC_CAT |
24.0 |
24.0 |
1386.0 |
O |
43.0 |
2023-02-24T23:05Z |
Additional measurement with more frames. |
Not modeled
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Carina Alden on 2023-02-26T16:38Z |
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