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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-03-24T15:38Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-03-24T15:38:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
DPL: CME exhibits dimpled front
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
Ha: Bright emission (likely H-alpha emission)
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: CME to the SW in SOHO LASCO C2/C3. Source is a large filament eruption seen just beyond the SW limb starting around 2024-03-24T13:56Z. Seen as ejecta in SDO AIA 304 and GOES SUVI 304. Ejecta and opening field lines in SDO AIA 171 and GOES SUVI 284 starting around 2024-03-24T13:20Z. Small amount of material seen ejecting from beyond the SW limb in SDO AIA 193 starting at 2024-03-24T15:03Z. This CME is not seen in STEREO A COR2 due to a data gap lasting from 2024-03-24T15:38Z to 2024-03-25T03:09Z.
Submitted on 2024-03-25T13:09Z 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 |
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CME Analysis
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M2M_CATALOG |
LE
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true |
Plane-of-sky |
NONE |
-63.0 |
585.0 |
C |
34.0 |
2024-03-24T22:27Z |
Plane of sky measurement since this CME is not seen in STEREO A COR2 due to a data gap lasting from 2024-03-24T15:38Z to 2024-03-25T03:09Z. Measurement of the bulk. Eruption appears so far out of the ecliptic in UV imagery that the Plane-of-sky fit is rather good. |
Not modeled
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Hannah Hermann on 2024-03-25T13:11Z |
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