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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2022-07-08T20:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2022-07-08T20:48:00-CME-001 (version 1)
Source Location: N20E40
Active Region Number: 13053
Note Keyword:
3P: 3-part structure CME
HAL: Halo CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
EUVW: EUV Wave
Morphology Keyword:
F: Flux Rope
Note: An eruption associated with the long-duration M2.5-class solar flare which occurred near N20E40. The CME presents itself as a faint halo in SOHO/C3 imagery and possibly a halo in Stereo-A/COR2A imagery with a bulk component mostly to the east in all available coronagraph imagery. The eruption as seen in coronal imagery is relatively unimpressive with mostly bright post-eruptive arcades and an EUV wave that traverses north and west of the source region best seen in SDO AIA 211 imagery.
Submitted on 2022-07-09T13:02Z by Chris
Stubenrauch
A Notification with ID
20220709-AL-002 was sent on 2022-07-09T15:16Z
A Notification with ID
20220709-AL-004 was sent on 2022-07-09T21:44Z
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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, earlier measurements are marked as false when new or more accurate measurements are made. This is a helpful flag if you would like to download only one most accurate CME analysis per CME |
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 |
-33.0 |
2.0 |
735.0 |
C |
47.0 |
2022-07-09T00:14Z |
A measurement of the CME bulk associated with this eruption. |
1: Result 1 (2.0 AU)
Earth = 2022-07-11T07:56Z
(PE: -1.4 h)
STEREO A = 2022-07-11T04:12Z
(PE: 11.7 h)
STEREO B = 2022-07-11T19:55Z
Parker Solar Probe = 2022-07-10T23:00Z
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Chris Stubenrauch on 2022-07-11T15:07Z |
CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
-24.0 |
6.0 |
1110.0 |
O |
47.0 |
2022-07-08T23:26Z |
A third measurement of the faintest shock front visible in all coronagraph imagery. |
Not modeled
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Chris Stubenrauch on 2022-07-09T13:32Z |
CME Analysis
|
M2M_CATALOG |
SH
|
false |
SWPC_CAT |
-21.0 |
6.0 |
1287.0 |
O |
49.0 |
2022-07-08T23:06Z |
A measurement of the faintest, fastest halo feature that is seen in SOHO and Stereo-A running difference imagery which quickly exits the Stereo-A field of view. This is a possible upper bound of the CME speed as it is uncertain whether this feature is associated with the halo. |
Not modeled
|
Chris Stubenrauch on 2022-07-09T13:13Z |
CME Analysis
|
M2M_CATALOG |
COR
|
false |
SWPC_CAT |
-56.0 |
3.0 |
707.0 |
C |
17.0 |
2022-07-09T00:31Z |
A measurement of the bulk of the CME. |
Not modeled
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Chris Stubenrauch on 2022-07-09T13:12Z |
CME Analysis
|
M2M_CATALOG |
LHB
|
false |
SWPC_CAT |
-41.0 |
3.0 |
941.0 |
C |
43.0 |
2022-07-09T00:23Z |
A measurement of the left-hand boundary of the CME, but wide enough to incorporate some aspects of the halo feature. |
Not modeled
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Chris Stubenrauch on 2022-07-09T13:16Z |
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