DONKI: Menu Page
Go to:
|
DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-13T09:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-05-13T09:12:00-CME-001 (version 1)
Source Location: S25W75
Active Region Number: 13664
Note Keyword:
3P: 3-part structure CME
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Full asymmetric halo CME seen to the SW in all three coronagraphs. Source is a large eruption and several M-class flares from Active Region 13664, including a long-duration M4.9 flare associated with the post-eruptive arcades. Widely opening field lines and a rising loop of ejecta seen starting at 2024-05-13T08:10Z in SDO AIA 193/171. Ejecta and post-eruptive brightening and arcades seen at 08:43Z in SDO AIA 131/304. Post eruptive arcades seen at 11:15Z in SDO AIA 171/193/304.
Submitted on 2024-05-13T13:22Z by Hannah
Hermann
A Notification with ID
20240513-AL-012 was sent on 2024-05-13T19:09Z
|
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 |
72.0 |
-36.0 |
1456.0 |
O |
49.0 |
2024-05-13T11:53Z |
Measurement of the BULK using source location seen in UV imagery, which also indicates some southern deflection, and best stereoscopic fit between coronagraphs. |
1: Result 1 (2.0 AU)
Mars = 2024-05-16T18:09Z
OSIRIS-APEX = 2024-05-16T03:29Z
Parker Solar Probe = 2024-05-14T19:15Z
STEREO A = 2024-05-16T04:00Z
2: Result 2 (5.5 AU)
Mars = 2024-05-16T18:40Z
Parker Solar Probe = 2024-05-14T19:14Z
OSIRIS-APEX = 2024-05-16T04:00Z
STEREO A = 2024-05-16T04:00Z
|
Hannah Hermann on 2024-05-15T19:40Z |
CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
26.0 |
-12.0 |
1935.0 |
O |
50.0 |
2024-05-13T11:15Z |
Measurement of the SHOCK of the CME using best fit between SOHO LASCO C3 and STEREO A COR2 coronagraphs. |
1: Result 1 (2.0 AU)
Earth = 2024-05-14T21:36Z
(PE: -20.6 h)
Lucy = 2024-05-16T13:29Z
STEREO A = 2024-05-14T19:11Z
|
Hannah Hermann on 2024-05-15T19:40Z |
|
All directly linked activities: |
|
|
Comments by users: |
0 comment received. |
|