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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-10-11T23:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2023-10-11T23:36:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
FOV: Front Bright front; may be evidence of pileup
OFL: Outflowing material at the back of the CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright CME visible in the east of SOHO LASCO C2/C3 and STEREO A COR2. The source eruption is seen as rapidly opening field lines in SDO AIA 171/193/304. The source location may be an active region just beyond the east limb, potentially one of a number of active regions that rotated off of the Earth-facing disk around 2023-09-30, including old AR 3435, which produced multiple M-class flares before rotating beyond the west limb around 2023-09-30.
Version 1 submitted on 2023-10-12T12:54Z by Mary Aronne
A Notification with ID
20231012-AL-001 was sent on 2023-10-12T13:20Z
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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) |
Measured On |
Submitted By |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-110.0 |
11.0 |
888.0 |
C |
36.0 |
2023-10-12T03:46Z |
Longitude based on source location just beyond the east limb, but there is some uncertainty in this measurement because the eruption cannot be seen on the disk. This longitude may vary by approximately +/- 10 degrees. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2023-10-13T04:52Z
Solar Orbiter = 2023-10-12T17:37Z
2: Result 2 (5.5 AU)
Parker Solar Probe = 2023-10-13T04:59Z
Solar Orbiter = 2023-10-12T17:37Z
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2023-10-12T12:55Z |
Mary Aronne on 2023-10-12T12:55Z |
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