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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-01-08T13:25Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-01-08T13:25:00-CME-001 (version 1)
Source Location: S26E45
Active Region Number: 13540
Note Keyword:
Faint: Faint event; may affect type assignment
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
Morphology Keyword:
F: Flux Rope
Note: Extremely faint CME first seen to the SE in SOHO LASCO C2. Extremely faint empty cavity also seen in C3. Leading edge appears brighter in STEREO A COR2 than in SOHO LASCO imagery. Source is on the Earth-facing disk. Opening field lines and dimming seen at S26E40-50 in SDO AIA 171/193 starting at 2024-01-08T12:06Z. Eruption of some, but not all, material from a small filament at S30E50 seen in SDO AIA 304 starting at 2024-01-08T11:51Z. Post-eruptive arcades seen forming at 2024-01-08T13:06Z located at S26E40-50 in SDO AIA 193. Source is in the vicinity of AR 13540 and 13541 (S17E40 and S20E36, respectively).
Submitted on 2024-01-08T20:57Z 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, 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 |
-44.0 |
-32.0 |
571.0 |
C |
31.0 |
2024-01-08T19:05Z |
Measurement of faint leading edge using source location on disk and best fit between coronagraphs. Leading edge becomes too diffuse to track after about ten frames in SOHO LASCO C3. |
1: Result 1 (2.0 AU)
Solar Orbiter = 2024-01-11T20:00Z
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Hannah Hermann on 2024-01-08T21:00Z |
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