DONKI: Menu Page
Go to:
|
DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-09-02T19:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
GOES: CCOR-1
Activity ID: 2026-09-02T19:36:00-CME-001 (version 3)
Source Location: N12E90
Active Region Number: 14524
Note Keyword:
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
Ha: Bright emission (likely H-alpha emission)
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright CME visible to the NE in SOHO LASCO C2, C3 and GOES CCOR-1 imagery. This CME is not visible in STEREO A COR2 imagery due to a data gap. The source of this CME is an M3.0 flare from an unnumbered region just beyond the NE limb. It is possible this is the returning region 14507 (N04) which rotated off of the Earth-facing disk on 2026-08-21. This long duration flare is associated with visible moving/opening field lines in SDO/AIA 193, 171, 211, GOES SUVI 304 and 284 starting around 2026-09-02T19:00Z. It is also associated with a filament eruption (best seen in GOES SUVI 304 starting around 2026-09-02T19:08Z), EUV wave (best seen in SDO/AIA 193 starting around 2026-09-02T19:27Z), and post-eruptive arcades visible in SDO/AIA 193 and 171 starting around 2026-09-02T21:00Z. There may also be H-alpha emission visible within SOHO LASCO C2 & C3 imagery.
Version 1 submitted on 2026-09-02T21:50Z by Carina Alden
Version 2 submitted on 2026-09-03T12:02Z by Elizabeth Juelfs
Version 3 submitted on 2026-09-03T15:08Z by Melissa Kane
A Notification with ID
20260902-AL-002 was sent on 2026-09-02T22:27Z
|
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 |
LE
|
true |
SWPC_CAT |
-90.0 |
27.0 |
1038.0 |
O |
35.0 |
2026-09-02T22:53Z |
BULK parameters based on best fit using SOHO LASCO C2, C3, and GOES CCOR-1 imagery. There may be some uncertainty with these parameters due to limited stereoscopic viewpoints. |
1: Result 1 (2.0 AU)
Europa Clipper = 2026-09-06T12:00Z
|
2026-09-02T21:41Z |
Carina Alden on 2026-09-02T21:52Z |
|
CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
-50.0 |
22.0 |
1323.0 |
O |
39.0 |
2026-09-02T22:03Z |
SHOCK parameters based on best fit using SOHO LASCO C2, C3, and GOES CCOR-1 imagery. There may be some uncertainty with these parameters due to limited stereoscopic viewpoints. |
1: Result 1 (2.0 AU)
Earth = 2026-09-05T18:00Z
Europa Clipper = 2026-09-04T20:47Z
OSIRIS-APEX = 2026-09-05T08:37Z
Juice = 2026-09-06T06:00Z
Solar Orbiter = 2026-09-04T02:00Z
|
2026-09-02T21:49Z |
Carina Alden on 2026-09-02T21:54Z |
|
All directly linked activities: |
|
|
|
| Comments by users: |
| 0 comment received. |
|
CCMC DONKI