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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-04-14T18:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2025-04-14T18:12:00-CME-001 (version 1)
Note Keyword:
Faint: Faint event; may affect type assignment
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
Note: CME first visible to the S in SOHO LASCO C2 starting at 2025-04-14T18:12Z in white light. CME is visible starting a few frames earlier at 2025-04-14T17:36Z in running difference imagery. This CME is also seen to the S in SOHO LASCO C3 but is partially obscured by the pylon. The source of this CME is possibly far-sided. There is not a good source candidate on the Earth-facing disk, but there is some very faint field line movement from on or beyond the S limb best seen in SDO AIA 171 beginning around 2025-04-14T15:42Z. The faint field line movement can also be seen in GOES SUVI 284. Another less likely source candidate is some minor movement starting around 2025-04-14T16:39Z best seen in SDO AIA 193 about S20E10.
Submitted on 2025-04-14T22:26Z by Elizabeth
Juelfs
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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 |
Plane-of-sky |
NONE |
-83.0 |
374.0 |
S |
25.0 |
2025-04-15T03:35Z |
Plane-of-sky measurement based on running difference imagery from SOHO LASCO C2. CME is partially visible in C3 but is too obscured by the the pylon to get a good measurement. Plane-of-sky measurement chosen due to lack of definitive source candidate. |
Not modeled
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Elizabeth Juelfs on 2025-04-14T22:29Z |
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