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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-11-19T21:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2023-11-19T21:24:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: Filament eruption seen to the N in all coronagraphs. Source is a filament over the high NE limb, first seen erupting over the limb at 2023-11-19T20:49Z in SDO AIA 304 and GOES SUVI 304. Additionally observed in SDO AIA 171/193/211 as moving field lines at the same time. As the filament source is far-sided, we do not observe the source longitude, but it is estimated to span around E120-E160 at a high latitude prior to erupting. During the eruption, a piece of the filament lags behind and may be responsible for a separate CME: 2023-11-20T00:12Z shortly after.
Submitted on 2023-11-20T20:03Z by Tony
Iampietro
No Notification has been sent for this activity yet.
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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 |
Plane-of-sky |
NONE |
79.0 |
505.0 |
C |
37.0 |
2023-11-20T04:51Z |
Plane-of-sky measurement as we do not observe the source of this filament erupting on the far-side of the disk over the NE limb. A follow-up measurement will be done to try sourcing a longitude in the range of E120-E160, but this is a high-latitude eruption regardless. |
Not modeled
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Tony Iampietro on 2023-11-20T20:09Z |
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