CCMC DONKI
Go to:
|
Interplanetary Shock (or CME Arrival)
Catalog: M2M_CATALOG Location: Earth Event Time: 2025-10-17T09:32Z ( ACE: MAG ) Quality of ICME Signature: 1 (lacks some signatures) Note: Characterized by a sudden increase in B-total from about 6 nT to about 12 nT, and peaking at 13 nT. Smooth rotation in the B-field components is observed. The sudden increase in B-total is immediately preceded by an increase in density from about 10cc to about 35cc, and has remained elevated at about 20cc for several hours since then. Solar wind speed has no significant increase, remaining around 390 km/s. Temperature has no notable increase. This signature was partially captured by DSCOVR after a data gap in DSCOVR lasting from 2025-10-17T08:52Z to 2025-10-17T10:58Z. The discontinuity seen in the magnetic field (Bz and Bx components) around 2025-10-17T13:15Z could indicate the arrival of the later (possibly the 2025-10-13T13:53Z) CME in what is likely a combined arrival of two CMEs (possibly the 2025-10-13T06:24Z and 2025-10-13T13:53Z CMEs). Version 1 submitted on 2025-10-17T11:59Z by Hannah Hermann Version 2 submitted on 2025-10-17T13:31Z by Hannah Hermann Version 3 submitted on 2025-10-17T15:50Z by Anna ChulakiA Notification with ID 20251017-AL-001 was sent on 2025-10-17T13:41Z |
||
All directly linked activities: |
||
|
||
| Comments by users: | ||
| 0 comment received. |
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