DONKI: Menu Page
Go to:
|
DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2022-04-29T07:38Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2022-04-29T07:38:00-CME-001 (version 3)
Source Location: N25W40
Active Region Number: 12996
Note Keyword:
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
DIM: Dimming
Morphology Keyword:
Note: Source is the eruption from AR 2996 (N25W40) starting around 2022-04-29T07:21Z seen in SDO AIA 131, 171, 193, and 304. Also visible on the NW limb of STA EUVI 195 around the same time. Post eruptive loops and dimming happens around 08:00Z. Associated with the M1.2 flare peaking at 07:30 from AR 2996.
Submitted on 2022-04-29T16:37Z by Mattie
Anastopulos
A Notification with ID
20220429-AL-003 was sent on 2022-04-29T13:25Z
A Notification with ID
20220429-AL-004 was sent on 2022-04-29T16:48Z
A Notification with ID
20220429-AL-005 was sent on 2022-04-29T18:00Z
A Notification with ID
20220430-AL-001 was sent on 2022-04-30T12:35Z
|
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 |
SH
|
true |
SWPC_CAT |
37.0 |
21.0 |
1397.0 |
O |
48.0 |
2022-04-29T09:53Z |
This measurement includes the back-filled SOHO LASCO C3 imagery. Limited imagery is available for STEREO A COR2. Speed measurements range from ~1300 km/s to ~1600 km/s tracking the shock front. |
1: Result 1 (2.0 AU)
Earth = 2022-05-01T04:05Z
Mars = 2022-05-02T07:26Z
OSIRIS-REx = 2022-05-01T23:01Z
STEREO B = 2022-05-01T03:14Z
Parker Solar Probe = 2022-05-01T01:30Z
STEREO A = 2022-05-02T12:00Z
|
Mattie Anastopulos on 2022-04-29T15:47Z |
CME Analysis
|
M2M_CATALOG |
SH
|
false |
StereoCAT |
41.0 |
25.0 |
1570.0 |
O |
43.0 |
2022-04-29T09:41Z |
Preliminary speed measurements range from around 1200 km/s to 1600 km/s depending on the feature tracked. Lower speeds correspond to the leading edge and higher speeds correspond to tracking the shock front. |
Not modeled
|
Mattie Anastopulos on 2022-04-29T13:07Z |
|
All directly linked activities: |
|
|
Comments by users: |
0 comment received. |
|