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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2022-11-22T20:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2022-11-22T20:24:00-CME-001 (version 1)
Source Location: S13E11
Active Region Number: 13151
Note Keyword:
Source Signature Keyword:
FLR: Flare
DIM: Dimming
Morphology Keyword:
Note: This CME is visible to the SE in SOHO LASCO C2/C3 and STEREO A COR2 coronagraph imagery. The source is likely the eruption from AR 3151 (S13E11) starting around 2022-11-22T19:00Z as seen in SDO AIA 131, 171, 193, 304 and STEREO A EUVI 195 and 304 imagery. There is post eruptive dimming visible to the north of AR 3151 in SDO AIA 171 and 193 shortly after the eruption occurs. This eruption and subsequent CME is associated with C4.8 flare.
Submitted on 2022-11-23T07:19Z by Mattie
Anastopulos
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, 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 |
CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
-26.0 |
24.0 |
415.0 |
S |
17.0 |
2022-11-23T03:48Z |
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1: Result 1 (2.0 AU)
Solar Orbiter = 2022-11-25T07:00Z
STEREO A = 2022-11-25T18:00Z
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Anna Chulaki on 2022-11-23T17:47Z |
CME Analysis
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M2M_CATALOG |
LE
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false |
SWPC_CAT |
-26.0 |
-24.0 |
415.0 |
S |
17.0 |
2022-11-23T03:48Z |
The CME is partially obscured by the pylon in SOHO LASCO C3 imagery. Also, limited imagery was available for this measurement as there is a data gap in SOHO LASCO C2/C3. |
Not modeled
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Mattie Anastopulos on 2022-11-23T07:23Z |
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