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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-08-17T16:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-08-17T16:00:00-CME-001 (version 1)
Note Keyword:
GAP: Data gap
OVR: Event partially overlaps with another CME
Source Signature Keyword:
Morphology Keyword:
Note: This CME is visible to the north in SOHO LASCO C2, C3, and a few frames among a data gap in STEREO A COR2 data. The frames in STEREO A COR2 are fairly noisy during this event. The source of this CME could potentially be a filament eruption visible along the N/NW limb believed to be on the far-side of the sun as seen in SDO/AIA 304. There are a few fronts visible in the coronagraphs that appear associated with this eruption, this front is first seen starting around 16:00Z while an earlier much slower front is seen starting around 15:12Z.
Submitted on 2024-08-18T01:28Z by Carina
Alden
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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 |
-168.0 |
64.0 |
377.0 |
S |
26.0 |
2024-08-18T01:44Z |
Parameters are based on best fit of feature using the possible source with notable deflection to the NE. |
Not modeled
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Carina Alden on 2024-08-18T01:30Z |
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