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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-11T01:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-05-11T01:36:00-CME-001 (version 1)
Source Location: S17W47
Active Region Number: 13664
Note Keyword:
DPL: CME exhibits dimpled front
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
HAL: Halo CME
OFL: Outflowing material at the back of the CME
Source Signature Keyword:
FLR: Flare
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Ear-shaped bright partial halo CME with a very complex shape brighter bulk and a fainter somewhat asymmetric full halo shock. The CME is associated with the X5.8 flare and a significant eruption (massive dimming) and EUV wave seen in SDO 193.
Submitted on 2024-05-11T04:35Z by Anna
Chulaki
A Notification with ID
20240511-AL-009 was sent on 2024-05-11T04:50Z
A Notification with ID
20240511-AL-012 was sent on 2024-05-11T14:23Z
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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 |
51.0 |
0.0 |
1263.0 |
O |
51.0 |
2024-05-11T04:22Z |
Updated bulk parameters. The CME bulk appears to have an earlobe shape to it with a smoother loop towards the north and a messy front to the south. It is possible these fronts could be interpreted as two separate CMEs overlapping each other, however they travel together in white-light and difference imagery. |
1: Result 1 (2.0 AU)
Earth = 2024-05-13T04:59Z
Lucy = 2024-05-14T18:37Z
Mars = 2024-05-13T17:42Z
Parker Solar Probe = 2024-05-12T05:42Z
STEREO A = 2024-05-12T20:25Z
OSIRIS-APEX = 2024-05-13T04:00Z
2: Result 2 (2.0 AU)
Earth = 2024-05-13T07:34Z
Lucy = 2024-05-14T19:24Z
Mars = 2024-05-13T23:50Z
Parker Solar Probe = 2024-05-12T05:49Z
STEREO A = 2024-05-12T21:22Z
OSIRIS-APEX = 2024-05-13T08:00Z
3: Result 3 (2.0 AU)
Earth = 2024-05-13T12:23Z
Lucy = 2024-05-15T04:37Z
Mars = 2024-05-14T06:18Z
Parker Solar Probe = 2024-05-12T07:59Z
STEREO A = 2024-05-13T01:07Z
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Carina Alden on 2024-05-11T13:53Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
15.0 |
-2.0 |
1820.0 |
O |
48.0 |
2024-05-11T03:24Z |
This is a SHOCK measurement based on the best fit of shock features in SOHO LASCO C3 and STEREO A COR2. Due to the asymmetric shape of the shock front, this measurement leaves out a little bit of the north/northwestern portion of the shock front. |
1: Result 1 (2.0 AU)
Earth = 2024-05-12T11:13Z
Lucy = 2024-05-13T20:37Z
STEREO A = 2024-05-12T08:15Z
Parker Solar Probe = 2024-05-12T14:00Z
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Carina Alden on 2024-05-11T17:59Z |
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CME Analysis
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M2M_CATALOG |
LE
|
false |
SWPC_CAT |
47.0 |
-1.0 |
1372.0 |
O |
49.0 |
2024-05-11T04:15Z |
A very preliminary analysis based on a decent but imperfect fit with two coronagraphs and on the location of the associated flare. The shape of this front is so complex that it is difficult to get an ideal fit. The CME half-width is a guess. This analysis needs to be reevaluated. |
Not modeled
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Anna Chulaki on 2024-05-11T04:41Z |
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