DONKI Header

CCMC DONKI

DONKI: Menu Page

Go to:

DONKI: View SW Activity
Interplanetary Shock (or CME Arrival)
Catalog: M2M_CATALOG
Location: Earth
Event Time: 2025-09-21T15:54Z ( ACE: MAG )
All Detecting Spacecrafts:
ACE: MAG
ACE: SWEPAM
Activity ID: 2025-09-21T15:54:00-IPS-001 (version 1)
Quality of ICME Signature: -1 (unspecified)
Note: Characterized by an amplification of magnetic field components from 1nT at 2025-09-21T15:54Z to 19nT at 2025-09-22T11:09Z. A subsequent increase in speed is observed from ~280 km/s at 2025-09-21T19:44Z to ~420 at 2025-09-22T11:10Z. Additionally, a gradual increase in density is observed starting around 2025-09-21T07:00Z, reaching ~20 p/cc at 2025-09-22T00:05Z. An increase in temperature is observed later around 2025-09-22T09:45Z, which coincides with the arrival of the 2025-09-22 high speed stream. The source of this interplanetary shock is likely a corotating interaction region preceding the coronal hole high speed stream starting on 2025-09-22. The coronal hole high speed stream is associated with a northern coronal hole that reached the central meridian on 2025-09-18. This event is still developing and analysis is ongoing.
Version 1 submitted on 2025-09-22T11:36Z by Mattie Anastopulos
Version 2 submitted on 2025-09-25T14:34Z by Mary Aronne
Version 3 submitted on 2025-09-25T15:46Z by Anna Chulaki
	
A Notification with ID 20250922-AL-002 was sent on 2025-09-22T11:43Z

All directly linked activities:
2025-09-22T01:12:00-HSS-001


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