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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-05-13T00:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2023-05-13T00:12:00-CME-001 (version 1)
Source Location: N15W76
Active Region Number: 13296
Note Keyword:
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
Ha: Bright emission (likely H-alpha emission)
KEY: Keyhole-hole shaped CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright and fast CME West in all coronagraphs with the source the C9.1 class flare from AR 3296 (N15W76) close to the NW limb starting at 2023-05-12T23:53Z and peaking at 2023-05-13T00:45Z, as seen in SDO AIA and GOES SUVI imagery. Associated with a beautiful large prominence eruption seen in AIA/SUVI 304 starting at 2023-05-12T23:24Z; marked by post-eruptive arcades in AIA/SUVI 193/195 and in EUVI A 304/195 after the data gap.
Submitted on 2023-05-13T14:02Z by Anna
Chulaki
A Notification with ID
20230513-AL-001 was sent on 2023-05-13T15:25Z
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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
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true |
SWPC_CAT |
77.0 |
3.0 |
733.0 |
C |
37.0 |
2023-05-13T05:08Z |
Analysis of what appears to be the bulk of the CME in white light imagery in SOHO and STEREO coronagraphs. A good fit in swpc_cat corresponds to the longitude of the source of this CME (flare from AR 3296). |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2023-05-14T20:56Z
OSIRIS-REx = 2023-05-17T15:00Z
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Anna Chulaki on 2023-05-13T14:09Z |
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CME Analysis
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M2M_CATALOG |
SH
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false |
SWPC_CAT |
122.0 |
15.0 |
751.0 |
C |
45.0 |
2023-05-13T04:55Z |
Measurement of what appears to be the shock front of the CME, based not on the longitude of the source (C9 class flare) but on the best fit in SOHO and STEREO A coronagraphs. Yields much higher longitude (122 deg) than the longitude of the source (~76 deg). |
Not modeled
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Anna Chulaki on 2023-05-13T14:05Z |
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