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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-03-03T06:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-03-03T06:36:00-CME-001 (version 1)
Note Keyword:
DFL: Likely deflection of the event within the FOV
DPL: CME exhibits dimpled front
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
F: Flux Rope
Note: Fast, asymmetric CME seen to the NE in all coronagraphs. Source is a small filament eruption on or just beyond the E limb centered around N08, lifting off around 2024-03-03T05:54Z in SDO AIA 304 and GOES SUVI 304. Additionally observed as moving field lines in SDO AIA 171/193/211.
Submitted on 2024-03-03T20:29Z by Tony
Iampietro
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 |
-92.0 |
27.0 |
767.0 |
C |
24.0 |
2024-03-03T11:09Z |
Measurement of the brighter inner portion of this CME, using SOHO LASCO C3 and STEREO COR2A only as the filament shape is evolving rapidly in SOHO LASCO C2. The diffuse, asymmetric front of this CME prevented many later frames from being used well. The range for this CME is likely E90-E100. |
1: Result 1 (2.0 AU)
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Tony Iampietro on 2024-03-03T20:32Z |
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