DONKI: Menu Page
Go to:
|
DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-10-14T00:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-10-14T00:48:00-CME-001 (version 2)
Source Location: N25E70
Note Keyword:
3P: 3-part structure CME
FOV: Front Bright front; may be evidence of pileup
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
PEA: Post eruption arcade
FIL: Filament eruption
DIM: Dimming
Morphology Keyword:
F: Flux Rope
Note: Bright CME seen to the E in all three coronagraphs, followed by two also very bright fronts, one with H-alpha emission. This could be the shock front of a two-lobed CME (the two following fronts being bulk fronts). Its source is the large prominence eruption on/close to the NE limb starting to lift off around 2025-10-14T00:00Z, as seen in GOES SUVI 304 (starting to rise around 2025-10-13T23:00Z), with massive post-eruptive arcades seen in SUVI 304 and 195 centered around N25E70.
Version 1 submitted on 2025-10-14T13:29Z by Anna Chulaki
Version 2 submitted on 2025-10-14T16:56Z by Anna Chulaki
A Notification with ID
20251014-AL-001 was sent on 2025-10-14T21:07Z
|
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) |
Measured On |
Submitted By |
|
CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
-78.0 |
9.0 |
874.0 |
C |
30.0 |
2025-10-14T05:23Z |
Analysis based on the fit of the front with two coronagraphs (SOHO LASCO C2/C3 and STEREO A COR2) and somewhat confirmed by the approximate location of the post-eruptive arcades (N25E70). |
1: Result 1 (2.0 AU)
BepiColombo = 2025-10-14T23:34Z
Parker Solar Probe = 2025-10-15T07:21Z
|
|
Anna Chulaki on 2025-10-14T17:34Z |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-78.0 |
6.0 |
667.0 |
C |
28.0 |
2025-10-14T06:54Z |
Analysis of this (secondary, likely bulk) bright front following the possible shock front, based on the fit with two coronagraphs (SOHO LASCO C2/C3 and STEREO A COR2), confirmed by the approximate location of the post-eruptive arcades following the filament eruption. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-10-15T03:46Z
Parker Solar Probe = 2025-10-15T12:40Z
2: Result 2 (2.0 AU)
BepiColombo = 2025-10-15T01:32Z
Parker Solar Probe = 2025-10-15T12:53Z
Mars = 2025-10-19T00:00Z
3: Result 3 (5.5 AU)
BepiColombo = 2025-10-15T01:09Z
Parker Solar Probe = 2025-10-15T12:33Z
Mars = 2025-10-19T00:00Z
Psyche = 2025-10-20T00:00Z
|
|
Anna Chulaki on 2025-10-14T17:34Z |
|
CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
-73.0 |
11.0 |
837.0 |
C |
34.0 |
2025-10-14T05:35Z |
Preliminary analysis based on SOHO LASCO C2/C3, STEREO A COR2, and GOES CCOR-1 in SWPC_CAT. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-10-15T00:48Z
Parker Solar Probe = 2025-10-15T08:02Z
Mars = 2025-10-18T10:00Z
2: Result 2 (5.5 AU)
BepiColombo = 2025-10-15T00:28Z
Parker Solar Probe = 2025-10-15T07:57Z
Psyche = 2025-10-19T14:00Z
Mars = 2025-10-18T10:00Z
|
|
Mary Aronne on 2025-10-17T12:38Z |
|
All directly linked activities: |
| No Linked Activity Found. |
|
| Comments by users: |
| 0 comment received. |
|
CCMC DONKI