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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-06-10T23:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-06-10T23:36:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
DFL: Likely deflection of the event within the FOV
DPL: CME exhibits dimpled front
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
OVR: Event partially overlaps with another CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
F: Flux Rope
FS: Flux Rope and Shock Candidate
Note: Wide filament eruption seen to the SW in all coronagraphs. Source is a filament eruption from the far-side of the disk, observed best as the filament material itself in SDO AIA 304 launching around 2024-06-10T22:30Z from around S30-S40. The filament material appears to be closer to the limb, but is accompanied by a wider far-sided field line movement in SDO AIA 171/193/211 that appears further around the limb. This is corroborated by the fit in swpc_cat between SOHO and STEREO coronagraphs not working unless longitudes >W130 were used. It appears that two fronts are traveling together from this front--perhaps the filament and field line movements--and are thus measured as one for this analysis.
Submitted on 2024-06-11T18:40Z by Tony
Iampietro
A Notification with ID
20240611-AL-002 was sent on 2024-06-11T23:32Z
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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 |
138.0 |
-41.0 |
914.0 |
C |
38.0 |
2024-06-11T03:35Z |
Measurement of the two apparent fronts from this eruption as one, requiring a right hand boundary measurement. Source initially appeared as the far-sided filament closer to the limb, perhaps W100-W110, but ultimately could not fit a triangulation between SOHO C2/C3 and STEREO COR2A unless we went W130-W145. |
1: Result 1 (2.0 AU)
OSIRIS-APEX = 2024-06-13T22:00Z
Solar Orbiter = 2024-06-13T16:00Z
2: Result 2 (5.5 AU)
OSIRIS-APEX = 2024-06-13T22:00Z
Solar Orbiter = 2024-06-13T16:00Z
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Tony Iampietro on 2025-03-12T16:56Z |
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| No Linked Activity Found. |
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