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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-10-25T14:01Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2023-10-25T14:01:00-CME-001 (version 1)
Source Location: S17E80
Note Keyword:
Faint: Faint event; may affect type assignment
FF: Event fails/disappears before exiting COR2
GAP: Data gap
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
O: Other
U: Unknown
Note: Faint CME that becomes very diffuse with no distinct leading edge in the SOHO LASCO C2 field of view. This CME overlaps partially with the CME first seen at 2023-10-25T13:37Z. The source of this CME is seen as moving/opening field lines to the SE in SDO/AIA 193, 211, and GOES SUVI 284. There is also a clear brightening in SDO/AIA 304 as well as a low C-level flare best seen in SDO/AIA 131.
Submitted on 2023-10-26T20:24Z by Carina
Alden
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 |
-80.0 |
3.0 |
288.0 |
S |
32.0 |
2023-10-26T02:09Z |
CME is too faint to track into C3 beyond the first two frames. The front of the CME becomes too diffuse to track well in C2. There is no defining shape to the CME, but tracking the brightest portions of the CME yielded these parameters. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2023-10-28T08:00Z
Solar Orbiter = 2023-10-28T00:00Z
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Carina Alden on 2023-10-26T20:26Z |
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