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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-10-24T03:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-10-24T03:48:00-CME-001 (version 1)
Source Location: S17E68
Active Region Number: 13869
Note Keyword:
3P: 3-part structure CME
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Partial halo CME visible to the SE in SOHO LASCO C2/C3 and STEREO A COR2. The source is an X3.3 flare starting at 2024-10-24T03:30Z from AR 3869 (approx. S17E68). Brightening and post eruptive arcades are observed in SDO AIA 131/171/193/335, EUV wave seen in SDO AIA 193, and opening field lines are best seen in SDO AIA 171/193. The eruption is also seen from STEREO A EUV 195/304.
Submitted on 2024-10-24T12:08Z by Mary
Aronne
A Notification with ID
20241024-AL-003 was sent on 2024-10-24T12:57Z
A Notification with ID
20241024-AL-004 was sent on 2024-10-24T22:29Z
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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 |
-54.0 |
-24.0 |
1606.0 |
O |
48.0 |
2024-10-24T05:57Z |
BULK measurement based on source location and the best fit between SOHO LASCO C2/C3 and STEREO A COR2 imagery in SWPC_CAT. |
1: Result 1 (2.0 AU)
Earth = 2024-10-26T02:00Z
(PE: -13.6 h)
Lucy = 2024-10-25T11:26Z
Parker Solar Probe = 2024-10-25T02:47Z
Solar Orbiter = 2024-10-24T23:53Z
OSIRIS-APEX = 2024-10-26T00:00Z
STEREO A = 2024-10-26T20:00Z
(PE: -14.4 h)
2: Result 2 (5.5 AU)
Earth = 2024-10-26T02:00Z
(PE: -13.6 h)
Lucy = 2024-10-25T11:31Z
Parker Solar Probe = 2024-10-25T02:40Z
Solar Orbiter = 2024-10-24T23:54Z
OSIRIS-APEX = 2024-10-26T00:00Z
STEREO A = 2024-10-26T20:00Z
(PE: -14.4 h)
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Tony Iampietro on 2024-10-24T17:54Z |
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CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
-36.0 |
-14.0 |
2006.0 |
R |
50.0 |
2024-10-24T05:37Z |
SHOCK MEASUREMENT triangulated between SOHO LASCO C3 and STEREO COR2A, following the outermost leading edge of the wider, fainter shock traveling ahead of the bulk. This notably does not capture the entire shock-like feature observed in both SOHO and STEREO coronagraphs in the SWPC_CAT measurement tool. This fit follows the leading edge of the shock best, cutting short from the widest portions of the partial halo. |
1: Result 1 (2.0 AU)
Earth = 2024-10-25T10:44Z
(PE: -28.8 h)
Lucy = 2024-10-25T03:31Z
Parker Solar Probe = 2024-10-25T00:20Z
Solar Orbiter = 2024-10-24T18:16Z
Mars = 2024-10-28T08:00Z
OSIRIS-APEX = 2024-10-26T12:00Z
STEREO A = 2024-10-26T00:00Z
(PE: -34.4 h)
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Tony Iampietro on 2024-10-24T16:51Z |
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