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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-01-27T15:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-01-27T15:12:00-CME-001 (version 1)
Note Keyword:
Faint: Faint event; may affect type assignment
GAP: Data gap
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Wide CME visible to the east in SOHO LASCO C2/C3. Not visible in STEREO A in COR2 in real-time due to a data gap. The leading edge of the CME fades away quickly in SOHO LASCO C3 by around 2024-01-27T18:18Z. The source is on the far side. Opening field lines can be seen in SDO AIA 171/103 around 2024-01-27T14:55Z. Material can also be seen ejected beyond the east limb in GOES SUVI 304. A candidate region for the source of this eruption is seen around longitude E150 in NSO GONG imagery on 2024-01-27.
Submitted on 2024-01-27T19:15Z by Mary
Aronne
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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 |
-151.0 |
11.0 |
441.0 |
S |
47.0 |
2024-01-27T23:05Z |
This measurement uses SOHO LASCO imagery only because no STEREO A coronagraph imagery was available. The longitude is approximated from possible far-sided source candidate as well as the fit of the best fit in the SWPC_CAT tool |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2024-01-30T00:34Z
2: Result 2 (2.0 AU)
Parker Solar Probe = 2024-01-30T00:14Z
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Mary Aronne on 2024-01-27T19:17Z |
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