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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-08-02T05:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-08-02T05:12:00-CME-001 (version 1)
Source Location: S14W88
Active Region Number: 13768
Note Keyword:
DFL: Likely deflection of the event within the FOV
FOV: Front Bright front; may be evidence of pileup
Ha: Bright emission (likely H-alpha emission)
OFL: Outflowing material at the back of the CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Wide, bright CME to the W in all coronagraphs. Source is an eruption from AR 3768 beginning around 2024-08-02T04:27Z, observed as wide field line movement, EUV wave, and a following post-eruptive arcade in SDO AIA 171/193/211/304 and GOES SUVI 171/195/284. Accompanied by a long-duration M7.4 flare which peaked at 2024-08-02T04:55Z, observed best in SDO AIA 131.
Submitted on 2024-08-02T13:42Z by Tony
Iampietro
A Notification with ID
20240802-AL-003 was sent on 2024-08-02T14:07Z
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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 |
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CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
82.0 |
-7.0 |
1164.0 |
O |
45.0 |
2024-08-02T08:19Z |
BULK measurement, triangulated between SOHO LASCO C3 and STEREO COR2A using the source of the eruption from AR 3768 around S14W88 as the source, finding a good fit slightly deflected eastward. This CME front is a bit lopsided to the northern end, so this fit best tracking the leading edge misses some material on the southern portion of the leading edge. |
1: Result 1 (2.0 AU)
Mars = 2024-08-05T06:14Z
OSIRIS-APEX = 2024-08-03T14:20Z
Solar Orbiter = 2024-08-04T21:00Z
STEREO A = 2024-08-05T05:00Z
2: Result 2 (5.5 AU)
Mars = 2024-08-05T05:24Z
OSIRIS-APEX = 2024-08-03T14:11Z
Juno = 2024-08-15T20:00Z
Solar Orbiter = 2024-08-04T21:00Z
STEREO A = 2024-08-05T05:00Z
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Tony Iampietro on 2024-08-02T13:45Z |
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