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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2022-12-04T01:25Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2022-12-04T01:25:00-CME-001 (version 3)
Note Keyword:
DFL: Likely deflection of the event within the FOV
GAP: Data gap
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
Note: This CME is seen faintly to the East in SOHO LASCO C2, C3, and STEREO A. The exact source is not clear, however a potential source of this CME is a filament eruption seen near N28E25 just NE of a large coronal hole starting around 2022-12-03T23:55Z, best seen in SDO/AIA 304 and 193. There is some deflection seen in SDO/AIA 094 to the SE of the eruption.
Submitted on 2022-12-05T01:17Z by Carina
Alden
A Notification with ID
20221204-AL-001 was sent on 2022-12-04T11:19Z
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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, earlier measurements are marked as false when new or more accurate measurements are made. This is a helpful flag if you would like to download only one most accurate CME analysis per CME |
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 |
-53.0 |
-9.0 |
545.0 |
C |
16.0 |
2022-12-04T06:40Z |
Analysis based on the best fit in two coronagraphs in SWPC_CAT since no clear source found, but the lat/lon fit the location of AR 3153 (S17E48) confirming the parameters |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2022-12-05T03:00Z
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Anna Chulaki on 2022-12-04T10:50Z |
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CME Analysis
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M2M_CATALOG |
LE
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false |
Plane-of-sky |
NONE |
-12.0 |
545.0 |
C |
24.0 |
2022-12-04T07:27Z |
There is likely deflection from the source location due to a large coronal hole to the SW of the eruption location. There is a data gap in STEREO A COR2 during this event, so the exact longitude is unknown. Therefore a plane-of-sky measurement was made. However, a measurement with a longitude of -30 degrees yielded a speed close to 855 km/s. Updated parameters may be provided once STEREO A COR2 science data becomes available. |
Not modeled
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Carina Alden on 2022-12-04T03:19Z |
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All directly linked activities: |
| No Linked Activity Found. |
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