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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-07-14T17:09Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2023-07-14T17:09:00-CME-001 (version 1)
Note Keyword:
COL: Possible collision with previous CME
FOV: Front Bright front; may be evidence of pileup
OVR: Event partially overlaps with another CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: The start time of this CME is based on STEREO A COR2 imagery due to real-time data gap in SOHO LASCO C2. Bright CME visible in the NE of SOHO LASCO C2/C3 and STEREO A COR2. The CME overlaps with at least one other CME in the field of view of the coronagraphs. The source is a filament eruption seen beyond the east limb as seen as filamentary material lifting off in GOES SUVI 104 around 2023-07-14T16:33Z. The footpoints of this filament were not visible on the disk in available EUV imagery.
Version 1 submitted on 2023-07-14T19:06Z by Mary Aronne
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) |
Measured On |
Submitted By |
|
CME Analysis
|
M2M_CATALOG |
LE
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true |
SWPC_CAT |
-121.0 |
28.0 |
682.0 |
C |
40.0 |
2023-07-14T21:51Z |
The longitude may vary by approximately +/- 10 degrees due to the uncertainty of the source location. The longitude is based off of source location somewhere just beyond the east limb with minor adjustments to fit the CME in the SWPC_CAT tool. Only one SOHO LASCO C3 image was available for this measurement. |
1: Result 1 (2.0 AU)
Mars = 2023-07-20T10:36Z
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2023-07-14T19:08Z |
Mary Aronne on 2023-07-14T19:08Z |
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