The 1.3-Year Variation in Solar Wind Speed and Geomagnetic Activity
Symposium E2.2, Coronal structure and dynamics near solar activity minimum ; 1998 ; Nagoya, Japan
Coronal structure and dynamics near solar activity minimum ; 9 ; 1939-1942
ADVANCES IN SPACE RESEARCH -OXFORD- ; 25 , 9
01.01.2000
4 pages
Held as part of the 32nd scientific assembly of the Committee on Space Research
Aufsatz (Konferenz)
Englisch
© Metadata Copyright the British Library Board and other contributors. All rights reserved.
The 1.3-Year Variation in Solar Wind Speed and Geomagnetic Activity
Online Contents | 2000
|Geomagnetic activity driven by solar wind turbulence
Online Contents | 2010
|Solar wind turbulence as a driver of geomagnetic activity
Online Contents | 2015
|