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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-06-11T23:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-06-11T23:12:00-CME-001 (version 6)
Note Keyword:
GAP: Data gap
HAL: Halo CME
SEP: Solar Energetic Particle event
Source Signature Keyword:
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Backsided partial halo CME first seen in SOHO LASCO C2 at 2024-06-11T23:12Z after a data gap; it is first seen in STEREO A COR2 coronagraph at 2024-06-12T00:38Z, after a large data gap which starts at 2024-06-11T12:53Z. Coronal signatures of this event include a backsided EUV wave seen as a fast opening/movement of field lines behind the west limb and a significant restructuring of magnetic field behind the limb seen in SDO AIA 171, 193, GOES SUVI 195, 171 and 304 imagery starting at 2024-06-11T22:39Z and in EUVI STEREO A 195 imagery after the data gap. The likely source of the CME is the old Active Region 3697 which is at S18W112 at the time of eruption.
Submitted on 2025-02-07T00:55Z by Anna
Chulaki
A Notification with ID
20240612-AL-005 was sent on 2024-06-12T05:41Z
A Notification with ID
20240612-AL-006 was sent on 2024-06-12T16:00Z
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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 |
113.0 |
26.0 |
1312.0 |
O |
48.0 |
2024-06-12T01:24Z |
UPDATED BULK measurement using source location approx. longitude of W112, several frames of C3, and the one frame of STEREO A COR2 that had some indication of the leading edge in the frame. |
1: Result 1 (2.0 AU)
Mars = 2024-06-15T00:59Z
OSIRIS-APEX = 2024-06-13T17:55Z
Parker Solar Probe = 2024-06-12T21:56Z
Solar Orbiter = 2024-06-14T01:35Z
2: Result 2 (5.5 AU)
Mars = 2024-06-15T01:29Z
OSIRIS-APEX = 2024-06-13T17:58Z
Parker Solar Probe = 2024-06-12T21:46Z
Solar Orbiter = 2024-06-14T02:05Z
Juno = 2024-06-26T06:00Z
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Hannah Hermann on 2024-06-12T13:27Z |
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CME Analysis
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M2M_CATALOG |
LE
|
false |
SWPC_CAT |
129.0 |
14.0 |
1019.0 |
O |
53.0 |
2024-06-12T02:07Z |
Very approximate analysis of this backsided event based on the best fit of what appears to be the bulk front of the CME (vs its wider shock). |
1: Result 1 (2.0 AU)
Mars = 2024-06-15T13:02Z
OSIRIS-APEX = 2024-06-14T00:25Z
Parker Solar Probe = 2024-06-13T03:28Z
Solar Orbiter = 2024-06-13T20:27Z
2: Result 2 (5.5 AU)
Mars = 2024-06-15T13:25Z
OSIRIS-APEX = 2024-06-14T00:24Z
Parker Solar Probe = 2024-06-13T03:15Z
Solar Orbiter = 2024-06-13T20:16Z
Juno = 2024-06-26T06:00Z
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Anna Chulaki on 2024-06-12T05:38Z |
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