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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2022-07-09T23:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2022-07-09T23:12:00-CME-001 (version 1)
Source Location: N15E10
Active Region Number: 13053
Note Keyword:
HAL: Halo CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
F: Flux Rope
J: Jet
Note: A complicated eruption consisting of a generally unimpressive flare/subsequent eruption in coronal imagery located around center-disk (N15E10) from AR3053. A fast jet of plasma is seen sharply deflecting towards the northwest due to the present of multiple coronal holes surrounding the active region, but SOHO/C2 coronagraph imagery shows what could be a faint, wider bulk associated with this eruption generally toward the northwest and an even fainter partial halo emanating generally to the west. It is uncertain whether the halo or bulk is associated with this center-disk eruption or another simultaneous eruption occurring off the Sun's western limb; moving field lines seen in SDO AIA 171 indicate this possibility. A Stereo-A COR2A outage at the time complicates the analysis of this event.
Submitted on 2022-07-10T19:56Z by Chris
Stubenrauch
A Notification with ID
20220711-AL-002 was sent on 2022-07-11T17:44Z
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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, 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 |
30.0 |
24.0 |
1258.0 |
O |
24.0 |
2022-07-10T01:36Z |
A measurement of the CME bulk generally headed toward the northwest in SOHO C2/C3 imagery. |
1: Result 1 (2.0 AU)
Earth = 2022-07-12T18:00Z
Parker Solar Probe = 2022-07-11T10:18Z
STEREO B = 2022-07-12T10:12Z
Mars = 2022-07-13T17:00Z
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Chris Stubenrauch on 2022-07-11T17:01Z |
CME Analysis
|
M2M_CATALOG |
COR
|
false |
SWPC_CAT |
48.0 |
24.0 |
1084.0 |
O |
22.0 |
2022-07-10T02:18Z |
A measurement of what is thought to be the bulk associated with the center-disk eruption and which is sharply deflected due to the presence of coronal holes near AR 3053. |
Not modeled
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Chris Stubenrauch on 2022-07-10T19:59Z |
CME Analysis
|
M2M_CATALOG |
SH
|
false |
SWPC_CAT |
16.0 |
20.0 |
1314.0 |
O |
45.0 |
2022-07-10T01:38Z |
A preliminary measurement of a faint shock feature that may possibly be associated with the center-disk eruption seen emanating to the west. It is unclear whether this feature is associated with this eruption or a simultaneous eruption behind the Sun's western limb. A Stereo A COR2A outage at this time complicated the analysis process of this feature. |
Not modeled
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Chris Stubenrauch on 2022-07-10T20:01Z |
CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
12.0 |
13.0 |
963.0 |
C |
45.0 |
2022-07-10T02:11Z |
This CME analysis is very uncertain. This is a very faint halo in C2 and even fainter in C3 and no STEREO A COR2 imagery (b/c of a data gap in STEREO A COR2). The 45 degree half-width is the default, the CME is probably narrower since it is very faint and the associated eruption area is small. |
1: Result 1 (2.0 AU)
Earth = 2022-07-12T03:10Z
Mars = 2022-07-13T15:17Z
Parker Solar Probe = 2022-07-11T10:42Z
STEREO A = 2022-07-12T06:54Z
STEREO B = 2022-07-12T06:04Z
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Chris Stubenrauch on 2022-07-11T17:20Z |
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