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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-01-06T17:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-01-06T17:36:00-CME-001 (version 1)
Source Location: N25E40
Note Keyword:
3P: 3-part structure CME
COL: Possible collision with previous CME
GAP: Data gap
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
Morphology Keyword:
F: Flux Rope
Note: CME seen to the northeast in SOHO LASCO C2/C3. Source is the second instance of dimming seen in SDO AIA 193, located at E45 and stretching from N25-N35, starting at 2024-01-06T16:20Z. Source also includes the lovely rising loop seen in SDO AIA 171, which is first visible off the NE limb at about 2024-01-06T15:30Z with field line movement at the suspected footpoints on the disk at N25E45 and N25E35. Post-eruptive arcades seen starting at 2024-01-06T18:48Z between the two suspected footpoints. There was no STEREO A COR2 imagery available for this CME due to a large data gap from 2024-01-06T09:23Z to 2024-01-07T04:09Z.
Submitted on 2024-01-07T20:46Z by Hannah
Hermann
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 |
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CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
-41.0 |
26.0 |
451.0 |
S |
36.0 |
2024-01-07T02:10Z |
Measurement using source location observed in UV imagery (around N25E40) and best fit in SOHO LASCO C2/C3 difference imagery as the CME propagated through the fields of view. Measurement matches very well with suspected source location. No STEREO A imagery available for this measurement due to a data gap lasting from 2024-01-06T09:23Z to 2024-01-07T04:09Z. |
1: Result 1 (2.0 AU)
Earth = 2024-01-10T01:00Z
Solar Orbiter = 2024-01-09T22:52Z
Psyche = 2024-01-11T07:00Z
STEREO A = 2024-01-10T00:00Z
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Hannah Hermann on 2024-01-07T20:48Z |
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