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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-06-10T18:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-06-10T18:36:00-CME-001 (version 1)
Source Location: S18W96
Active Region Number: 13697
Note Keyword:
DPL: CME exhibits dimpled front
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
Ha: Bright emission (likely H-alpha emission)
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Wide CME seen to the W in SOHO LASCO C2/C3, not in STEREO COR2A due to a lengthy data gap over this period. The source is an occulted M9.5 flare from AR 3697 (estimated around the limb ~S18W96 at the time) which peaked at 2024-06-10T18:40Z, best observed in SDO AIA 131. Also observed as field line movement and an EUV wave in SDO AIA 171/193/211 starting around 2024-06-11T17:54Z, with post-eruptive arcades forming after the flare peak.
Submitted on 2024-06-11T13:12Z by Tony
Iampietro
A Notification with ID
20240611-AL-001 was sent on 2024-06-11T13:42Z
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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 |
96.0 |
11.0 |
1142.0 |
O |
43.0 |
2024-06-10T21:34Z |
BULK measurement using only SOHO C3 imagery, due to a STEREO COR2A data gap. Source longitude of AR 3697 (S18W96) used as a basis, finding a northward deflection with a good fit. |
1: Result 1 (2.0 AU)
Mars = 2024-06-14T03:53Z
OSIRIS-APEX = 2024-06-12T19:04Z
Parker Solar Probe = 2024-06-11T21:42Z
Solar Orbiter = 2024-06-13T12:00Z
2: Result 2 (5.5 AU)
Mars = 2024-06-14T04:22Z
OSIRIS-APEX = 2024-06-12T19:02Z
Parker Solar Probe = 2024-06-11T21:32Z
Solar Orbiter = 2024-06-13T12:00Z
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Tony Iampietro on 2024-06-11T13:31Z |
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CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
139.0 |
3.0 |
1352.0 |
O |
48.0 |
2024-06-10T21:08Z |
SHOCK measurement using only SOHO C3 imagery, due to a STEREO COR2A data gap. Source longitude of AR 3697 (S18W96) used as a basis, ultimately fitting much better around W139. |
1: Result 1 (2.0 AU)
OSIRIS-APEX = 2024-06-12T14:02Z
Parker Solar Probe = 2024-06-12T04:08Z
Solar Orbiter = 2024-06-12T08:14Z
2: Result 2 (5.5 AU)
OSIRIS-APEX = 2024-06-12T14:24Z
Parker Solar Probe = 2024-06-12T04:27Z
Solar Orbiter = 2024-06-12T08:04Z
Juno = 2024-06-22T09:00Z
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Tony Iampietro on 2024-06-11T13:31Z |
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