DONKI: Menu Page
Go to:
|
DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-11-14T08:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-11-14T08:00:00-CME-001 (version 3)
Source Location: N24W71
Active Region Number: 14274
Note Keyword:
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
F: Flux Rope
L: Loop
Note: Asymmetric halo seen with bulk to the northwest with a faint halo-shaped shock in SOHO LASCO C2/LASCO C3 and GOES CCOR-1 with wider bulk seen to the north and northwest in STEREO A COR2A associated with an X4.0-class solar flare from AR14274 (N24W71). The eruption is characterized by brightening seen best in GOES SUVI 131 and as well in GOES SUVI 195 and GOES SUVI 284 imagery with a significant, rapid field line movement and darkening seen off the northwest limb around 2025-11-14T07:45Z.
Version 1 submitted on 2025-11-14T13:38Z by Chris Stubenrauch
Version 2 submitted on 2025-11-14T13:59Z by Chris Stubenrauch
Version 3 submitted on 2025-11-17T17:04Z by Mary Aronne
A Notification with ID
20251114-AL-008 was sent on 2025-11-14T13:56Z
A Notification with ID
20251114-AL-010 was sent on 2025-11-14T17:38Z
|
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 |
49.0 |
3.0 |
1082.0 |
O |
54.0 |
2025-11-14T11:11Z |
Measurement of the SHOCK feature using the best fit between several frames of SOHO LASCO C3, GOES CCOR-1, and STEREO A COR2. |
1: Result 1 (2.0 AU)
Earth = 2025-11-16T02:49Z
(PE: 1.3 h)
BepiColombo = 2025-11-14T19:34Z
OSIRIS-APEX = 2025-11-15T19:30Z
Solar Orbiter = 2025-11-15T19:13Z
STEREO A = 2025-11-16T03:02Z
(PE: 11.1 h)
|
|
Tony Iampietro on 2025-11-14T16:17Z |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
62.0 |
9.0 |
1534.0 |
O |
40.0 |
2025-11-14T10:40Z |
Measurement of the BULK using source location seen in available UV imagery and best fit between several frames of SOHO LASCO C2/C3, STEREO A COR2, and GOES CCOR-1. |
1: Result 1 (2.0 AU)
Earth = 2025-11-16T10:00Z
(PE: 8.5 h)
BepiColombo = 2025-11-14T20:07Z
OSIRIS-APEX = 2025-11-16T01:12Z
Solar Orbiter = 2025-11-15T20:41Z
STEREO A = 2025-11-15T20:37Z
(PE: 4.7 h)
2: Result 2 (5.5 AU)
Earth = 2025-11-16T10:00Z
(PE: 8.5 h)
BepiColombo = 2025-11-14T20:06Z
OSIRIS-APEX = 2025-11-16T01:46Z
Solar Orbiter = 2025-11-15T20:58Z
STEREO A = 2025-11-15T20:50Z
(PE: 4.9 h)
Juno = 2025-11-26T00:00Z
|
|
Hannah Hermann on 2025-11-14T14:57Z |
|
CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
70.0 |
22.0 |
1261.0 |
O |
45.0 |
2025-11-14T11:11Z |
Preliminary measurement of the bulk of the CME using limited SOHO LASCO C2/C3 frames and STEREO A COR2 out to 17 solar radii. |
Not modeled
|
2025-11-14T13:21Z |
Chris Stubenrauch on 2025-11-14T13:42Z |
|
All directly linked activities: |
|
|
|
| Comments by users: |
| 0 comment received. |
|
CCMC DONKI