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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-12-20T23:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-12-20T23:48:00-CME-001 (version 1)
Note Keyword:
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
GAP: Data gap
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
U: Unknown
Note: Narrow CME visible to the SW in SOHO LASCO C2/C3 and STEREO A COR2, directly following CME: 2024-12-21T21:12Z in the field of view of the coronagraphs. The potential source is near or beyond the west limb as seen in SDO AIA and STEREO A EUV imagery. In GOES SUVI 304, ejecta can be seen departing on the limb starting at 2024-12-20T23:00Z. Moving/opening field lines are also visible in GOES SUVI 195/284 and STEREO A EUV 195.
Submitted on 2024-12-21T18:50Z by Mary
Aronne
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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 |
CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
105.0 |
-19.0 |
303.0 |
S |
15.0 |
2024-12-21T11:16Z |
Measurement based on the best fit between SOHO LASCO C2/C3 and STEREO A COR2 imagery in SWPC_CAT as well as the potential source location. |
1: Result 1 (2.0 AU)
2: Result 2 (5.5 AU)
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Mary Aronne on 2024-12-21T18:51Z |
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