DONKI Header

CCMC DONKI

DONKI: Menu Page

Go to:

DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-09-03T05:38Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
GOES: CCOR-1
Activity ID: 2025-09-03T05:38:00-CME-001 (version 2)
Note Keyword:
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
L: Loop
Note: CME first seen to the NW in STEREO A COR2 starting at 2025-09-03T05:38Z. CME is also seen to NW in SOHO LASCO C2/C3 and GOES CCOR-1, but is partially obscured by the pylon. The source of this CME is most likely a filament eruption from the NW quadrant of the Earth-facing disk centered around N30W50. The filament can been seen rising off the disk is SDO AIA 304 beginning around 2025-09-03T00:31Z. The filament eruption can also be seen in STA EUVI 304 slightly N of center disk.
Version 1 submitted on 2025-09-03T13:54Z by Elizabeth Juelfs
Version 2 submitted on 2025-09-03T21:07Z by Melissa Kane
	
A Notification with ID 20250903-AL-001 was sent on 2025-09-03T15:59Z
A Notification with ID 20250903-AL-002 was sent on 2025-09-03T22:01Z

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 57.0 27.0 434.0 S 30.0 2025-09-03T12:15Z Updated bulk measurement based on best fit in SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1 using backfilled SOHO LASCO imagery that was previously unavailable. 1: Result 1 (2.0 AU)
STEREO A = 2025-09-06T08:00Z
Juice = 2025-09-05T12:00Z
2025-09-03T21:09Z Melissa Kane on 2025-09-03T21:09Z
CME Analysis M2M_CATALOG LE false SWPC_CAT 52.0 19.0 602.0 C 29.0 2025-09-03T10:10Z Measurement based on source location and fit in STEREO A COR2. 1: Result 1 (2.0 AU)
STEREO A = 2025-09-06T03:53Z
Juice = 2025-09-05T06:00Z
OSIRIS-APEX = 2025-09-06T20:00Z
2025-09-03T13:55Z Elizabeth Juelfs on 2025-09-03T13:55Z



All directly linked activities:
No Linked Activity Found.


Comments by users:
0 comment received.
Insert title here

The Moon to Mars Space Weather Analysis Office and other entities provide data to DONKI as a courtesy to the community.
By visiting this site, you acknowledge that you understand and agree to the Important Disclaimer Notice

If you are looking for the official U.S. Government forecast for space weather, please go to NOAA's Space Weather Prediction Center (https://swpc.noaa.gov). This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy