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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-10-03T12:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-10-03T12:48:00-CME-001 (version 2)
Source Location: S15W05
Active Region Number: 13842
Note Keyword:
DPL: CME exhibits dimpled front
Ha: Bright emission (likely H-alpha emission)
HAL: Halo CME
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Full halo CME observed in SOHO LASCO, and full halo directed slightly more eastward in STEREO COR2A. The source is an X9.0 flare from AR 3842 observed in many wavelengths but mainly SDO AIA 131, starting at 2024-10-03T12:08Z and peaking at T12:18Z. Also observed as an EUV wave and dimming in SDO AIA 171/193 and GOES SUVI 284, with surface brightening in SDO AIA 304.
Submitted on 2024-10-03T16:50Z by Tony
Iampietro
A Notification with ID
20241003-AL-004 was sent on 2024-10-03T17:08Z
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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
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
3.0 |
-20.0 |
822.0 |
C |
39.0 |
2024-10-03T16:43Z |
BULK measurement based on best fit between SOHO LASCO C2/C3 and STEREO A COR2 |
1: Result 1 (2.0 AU)
Earth = 2024-10-06T04:39Z
(PE: -2.3 h)
Lucy = 2024-10-06T03:54Z
STEREO A = 2024-10-05T22:13Z
(PE: 2.7 h)
Mars = 2024-10-07T10:00Z
2: Result 2 (5.5 AU)
Earth = 2024-10-06T03:43Z
(PE: -3.2 h)
Lucy = 2024-10-06T02:42Z
STEREO A = 2024-10-05T21:43Z
(PE: 2.2 h)
Juno = 2024-10-17T00:00Z
Mars = 2024-10-07T10:00Z
3: Result 3 (2.0 AU)
Earth = 2024-10-04T20:19Z
(PE: -34.6 h)
Lucy = 2024-10-04T19:23Z
STEREO A = 2024-10-05T20:44Z
(PE: 1.2 h)
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Tony Iampietro on 2024-10-03T17:26Z |
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CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
-3.0 |
-4.0 |
863.0 |
C |
53.0 |
2024-10-03T16:29Z |
SHOCK measurment triangulated between SOHO LASCO C2/C3 and STEREO COR2A. The shock front is notably wide with a "layered" appearance in both SOHO and STEREO with some apparent concentric fronts, along with being a bit "wider" than it was "taller" with an overall oval-shape in SOHO. The best fit between both shock fronts is presented here, though it does not capture 100% of the shock front which may be even wider. |
1: Result 1 (2.0 AU)
Earth = 2024-10-05T21:49Z
(PE: -9.1 h)
Lucy = 2024-10-05T16:59Z
Mars = 2024-10-07T01:21Z
STEREO A = 2024-10-05T16:34Z
(PE: -2.9 h)
Solar Orbiter = 2024-10-04T10:00Z
2: Result 2 (5.5 AU)
Earth = 2024-10-05T21:03Z
(PE: -9.9 h)
Lucy = 2024-10-05T15:54Z
Mars = 2024-10-07T01:13Z
STEREO A = 2024-10-05T16:04Z
(PE: -3.4 h)
Juno = 2024-10-16T22:00Z
Solar Orbiter = 2024-10-04T10:00Z
3: Result 3 (2.0 AU)
Earth = 2024-10-04T01:18Z
(PE: -53.6 h)
Lucy = 2024-10-04T00:37Z
Mars = 2024-10-05T01:39Z
STEREO A = 2024-10-03T20:22Z
(PE: -47.1 h)
Solar Orbiter = 2024-10-02T18:00Z
4: Result 4 (5.5 AU)
Earth = 2024-10-04T00:41Z
(PE: -54.2 h)
Lucy = 2024-10-03T23:45Z
Mars = 2024-10-05T01:31Z
STEREO A = 2024-10-03T19:52Z
(PE: -47.6 h)
Juno = 2024-10-15T08:00Z
Solar Orbiter = 2024-10-02T18:00Z
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Tony Iampietro on 2024-10-03T17:16Z |
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