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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-28T02:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-07-28T02:24:00-CME-001 (version 2)
Source Location: S08E10
Active Region Number: 13766
Note Keyword:
3P: 3-part structure CME
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Full halo CME visible in SOHO LASCO C2/C3 and towards the east in STEREO A COR2. The source is likely the M9.9 flare peaking at 2024-07-28T01:57Z from AR 3766 and/or the M7.8 flare directly preceding it from the same region. Dimming and EUV wave visible in SDO AIA 193 and 335 and GOES SUVI 284, post-eruptive arcades visible in SDO AIA 131/171/193. The eruption is also visible in STEREO A EUV imagery.
Submitted on 2024-07-28T13:06Z by Mary
Aronne
A Notification with ID
20240728-AL-006 was sent on 2024-07-28T22:16Z
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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 |
CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
1.0 |
-2.0 |
920.0 |
C |
45.0 |
2024-07-28T05:39Z |
SHOCK measurement of wider, fainter shock feature ahead of the leading edge of the CME. |
1: Result 1 (2.0 AU)
Earth = 2024-07-30T12:03Z
(PE: -25.7 h)
Lucy = 2024-07-31T16:39Z
Parker Solar Probe = 2024-07-29T13:29Z
STEREO A = 2024-07-30T04:28Z
(PE: -20.6 h)
Mars = 2024-08-02T00:00Z
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Mattie Anastopulos on 2024-07-28T21:48Z |
CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
3.0 |
5.0 |
559.0 |
C |
45.0 |
2024-07-28T08:26Z |
Updated bulk measurement based on the best fit between SOHO LASCO C3 and STEREO A COR2 coronagraph imagery. |
1: Result 1 (2.0 AU)
Earth = 2024-07-31T05:15Z
(PE: -8.5 h)
Lucy = 2024-08-01T13:16Z
Parker Solar Probe = 2024-07-30T02:58Z
STEREO A = 2024-07-30T20:57Z
(PE: -4.1 h)
Mars = 2024-08-02T02:00Z
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Mattie Anastopulos on 2024-07-28T21:47Z |
CME Analysis
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M2M_CATALOG |
LE
|
false |
SWPC_CAT |
1.0 |
4.0 |
557.0 |
C |
43.0 |
2024-07-28T08:02Z |
Measurement of leading edge of the CME based on source location and best fit between SOHO LASCO C2/C3 and STEREO A COR2 imagery in SWPC_CAT. |
1: Result 1 (2.0 AU)
Earth = 2024-07-31T07:14Z
(PE: -6.5 h)
Lucy = 2024-08-01T14:13Z
Parker Solar Probe = 2024-07-30T03:21Z
STEREO A = 2024-07-30T21:49Z
(PE: -3.3 h)
2: Result 2 (2.0 AU)
Earth = 2024-07-31T05:15Z
(PE: -8.5 h)
Lucy = 2024-08-01T13:06Z
Parker Solar Probe = 2024-07-30T02:37Z
STEREO A = 2024-07-30T21:08Z
(PE: -4.0 h)
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Mary Aronne on 2024-07-28T13:54Z |
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