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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2022-05-21T00:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2022-05-21T00:12:00-CME-001 (version 3)
Source Location: N18W31
Active Region Number: 13011
Note Keyword:
Faint: Faint event; may affect type assignment
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
BR: Brightening
Morphology Keyword:
F: Flux Rope
Note: The likely source is an eruption from AR3011 (N18W31) which was associated with a C5.2 class flare occurring around 2022-05-20T23:30Z. After the brightening, filament material is ejected to the north and west as seen in SDO AIA 304A. Soon after this eruption, a complex signature is observed in SOHO running difference imagery with a large, faint and fast shock on the order of >1000 km/s emanating to the north which may or may not be associated with this flare. A coronal hole located to the southwest of the active region(s) possibly producing the eruption may have deflected the ejecta in the northward and eastward directions.
Submitted on 2022-05-22T18:40Z by Chris
Stubenrauch
A Notification with ID
20220522-AL-001 was sent on 2022-05-22T18:37Z
A Notification with ID
20220522-AL-002 was sent on 2022-05-22T19:39Z
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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 |
COR
|
true |
SWPC_CAT |
25.0 |
28.0 |
569.0 |
C |
33.0 |
2022-05-21T05:47Z |
A measurement of the bulk of the CME outflow using only SOHO/C2 running difference imagery. |
1: Result 1 (2.0 AU)
Earth = 2022-05-24T11:00Z
STEREO B = 2022-05-24T05:34Z
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Chris Stubenrauch on 2022-05-22T17:49Z |
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CME Analysis
|
M2M_CATALOG |
COR
|
false |
SWPC_CAT |
48.0 |
26.0 |
487.0 |
S |
30.0 |
2022-05-21T07:03Z |
Upon analysis, there are two eruptions present in SOHO running difference imagery, only the first of which, a narrower event, correlates with the Stereo A/COR2A imagery. Thus, the CME of interest is only seen in SOHO imagery and the filamentary material is largely deflected to the north and west as seen in SDO AIA 304. There is also a weak shock front produced to the north in SOHO C2 running difference imagery on the order of 1000 km/s which may or may not be associated with this eruption. |
1: Result 1 (2.0 AU)
STEREO B = 2022-05-24T12:00Z
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Chris Stubenrauch on 2022-05-21T14:18Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
31.0 |
15.0 |
476.0 |
S |
10.0 |
2022-05-21T05:39Z |
A measurement of the earlier more narrow CME associated with this series of eruptions. |
Not modeled
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Chris Stubenrauch on 2022-05-21T19:02Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
false |
SWPC_CAT |
8.0 |
11.0 |
990.0 |
C |
21.0 |
2022-05-21T02:06Z |
A measurement incorporating the bright feature observed in a few frames of COR2A. |
Not modeled
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Chris Stubenrauch on 2022-05-22T16:10Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
false |
SWPC_CAT |
18.0 |
24.0 |
1175.0 |
O |
29.0 |
2022-05-21T02:38Z |
A measurement of the weakest and faintest shock associated with this eruption using only SOHO coronagraph imagery. |
Not modeled
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Chris Stubenrauch on 2022-05-22T16:11Z |
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