DONKI: Menu Page
Go to:
|
DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-01-30T18:09Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C3
Activity ID: 2023-01-30T18:09:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
Note: This CME is visible to the SW in STEREO A COR2 and SOHO LASCO C3 coronagraph imagery. The source is likely far-sided, but there is field line movement visible off the SW limb in SDO AIA 171 imagery starting around 2023-01-30T17:30Z.
Submitted on 2023-01-31T13:45Z by Mattie
Anastopulos
A Notification with ID
20230131-AL-001 was sent on 2023-01-31T16:58Z
|
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 |
LE
|
true |
SWPC_CAT |
149.0 |
-37.0 |
705.0 |
C |
40.0 |
2023-01-30T22:48Z |
Since the source is far-sided and there is no exact source location, the longitude was estimated based on the best fit between SOHO LASCO C3 and STEREO A COR2. Longitude may vary +/-10 degrees as a result. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2023-02-02T08:00Z
|
Mattie Anastopulos on 2023-01-31T13:48Z |
|
All directly linked activities: |
No Linked Activity Found. |
|
Comments by users: |
0 comment received. |
|