DONKI Header

CCMC DONKI

DONKI: Menu Page

Go to:

DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-10-14T01:38Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
GOES: CCOR-1
Activity ID: 2025-10-14T01:38:00-CME-001 (version 2)
Note Keyword:
COL: Possible collision with previous CME
FOV: Front Bright front; may be evidence of pileup
HAL: Halo CME
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
OFL: Moving/Opening field lines
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright, more northern, follow-up front to 2025-10-14T00:48Z CME front; looking more like a partial halo in STEREO A COR2 coronagraph. The CME visibly widens as it develops and seemingly becomes more northern with time. Its source is likely the same large prominence eruption off the E limb seen in GOES SUVI imagery that is the source of the 2025-10-14T00:48Z front.
Version 1 submitted on 2025-10-14T13:33Z by Anna Chulaki
Version 2 submitted on 2025-10-14T17:03Z 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 LE true SWPC_CAT -92.0 20.0 877.0 C 32.0 2025-10-14T06:10Z Very approximate reanalysis of this front with more imagery based on two coronagraph fit: SOHO LASCO C2/C3 and STEREO A COR2. 1: Result 1 (2.0 AU)
BepiColombo = 2025-10-15T00:36Z
Parker Solar Probe = 2025-10-15T09:42Z
2: Result 2 (5.5 AU)
BepiColombo = 2025-10-15T00:01Z
Parker Solar Probe = 2025-10-15T09:30Z
Psyche = 2025-10-19T18:00Z
3: Result 3 (2.0 AU)
BepiColombo = 2025-10-15T01:32Z
Parker Solar Probe = 2025-10-15T12:53Z
Mars = 2025-10-19T00:00Z
4: Result 4 (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 2025-10-14T17:05Z
CME Analysis M2M_CATALOG LE false SWPC_CAT -97.0 16.0 747.0 C 35.0 2025-10-14T06:26Z 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
Anna Chulaki on 2025-10-14T13:34Z



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