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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-02-09T13:23Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-02-09T13:23:00-CME-001 (version 3)
Source Location: S37W110
Active Region Number: 13575
Note Keyword:
COL: Possible collision with previous CME
HAL: Halo CME
OVR: Event partially overlaps with another CME
SEP: Solar Energetic Particle event
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Partial halo CME where the source is an X3.3 class flare from AR 3575 (S36W110) peaking at 2023-02-09T13:14Z and the associated eruption seen in AIA 193/171 and EUVI A 195 starting ~2024-02-09T3:30Z as an EUV wave mostly to the south on the visible disk, but extending to central meridian and as very fast wide opening of field lines and as bright post-eruptive arcades behind the SW limb.
Submitted on 2025-02-07T23:51Z by Anna
Chulaki
A Notification with ID
20240209-AL-003 was sent on 2024-02-09T14:28Z
A Notification with ID
20240209-AL-009 was sent on 2024-02-09T16:03Z
A Notification with ID
20240209-AL-011 was sent on 2024-02-09T19:34Z
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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
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
130.0 |
-24.0 |
2534.0 |
R |
48.0 |
2024-02-09T14:31Z |
Uncertain analysis of the faint wispy shock preceding the bulk front. This analysis does not include the wider halo feature associated with this CME that seems to be even more backsided, based on fitting it in swpc_cat. |
1: Result 1 (2.0 AU)
Mars = 2024-02-11T05:54Z
OSIRIS-APEX = 2024-02-10T05:40Z
Parker Solar Probe = 2024-02-10T16:00Z
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Anna Chulaki on 2024-02-10T12:42Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
110.0 |
-34.0 |
1754.0 |
O |
46.0 |
2024-02-09T15:11Z |
Analysis with additional coronagraph imagery. |
1: Result 1 (2.0 AU)
Mars = 2024-02-12T02:54Z
OSIRIS-APEX = 2024-02-10T12:49Z
Parker Solar Probe = 2024-02-11T13:30Z
2: Result 2 (5.5 AU)
Mars = 2024-02-12T03:11Z
OSIRIS-APEX = 2024-02-10T12:55Z
Lucy = 2024-02-14T02:00Z
Parker Solar Probe = 2024-02-11T13:30Z
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Anna Chulaki on 2024-02-14T16:48Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
110.0 |
-33.0 |
2226.0 |
R |
48.0 |
2024-02-09T14:50Z |
Initial analysis with only a couple early coronagraph frames, needs to be remeasured with more imagery. |
1: Result 1 (2.0 AU)
Mars = 2024-02-11T15:16Z
OSIRIS-APEX = 2024-02-10T08:26Z
Lucy = 2024-02-13T12:00Z
Parker Solar Probe = 2024-02-11T10:00Z
2: Result 2 (5.5 AU)
Mars = 2024-02-11T15:27Z
OSIRIS-APEX = 2024-02-10T08:28Z
Parker Solar Probe = 2024-02-11T10:00Z
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Anna Chulaki on 2024-02-10T12:37Z |
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