Abstract The results of the solar wind interaction with the local interstellar medium (LISM) theory are considered. The model is characterized by the presence of two shocks: a bow shock, a heliospheric shock, and a contact discontinuity. On the basis of the theoretical results and the Voyager data, the electron number density in LISM is estimated.
The interface between heliosphere and the local intersteller medium (LISM)
Advances in Space Research ; 6 , 2 ; 5-12
1986-01-01
8 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Penetration of the Galactic Cosmic Rays into the Heliosphere through LISM-Solar Wind Interface
Online Contents | 1997
|Penetration of the Galactic Cosmic Rays into the Heliosphere through LISM-Solar Wind Interface
British Library Conference Proceedings | 1997
|LISM Mission for SELENE Project
British Library Conference Proceedings | 2000
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