Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..716b&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Sept. 1986, p. 716-721) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Sept.-O
Astronomy and Astrophysics
Astronomy
2
Astronomical Models, Electron Density (Concentration), Heliosphere, Interstellar Space, Satellite Observation, Solar Wind, Hydrogen Atoms, Solar Activity Effects, Voyager 1 Spacecraft, Voyager 2 Spacecraft
Scientific paper
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 (bow shock and heliospheric shock) and the contact discontinuity. The theoretical results are compared with the Voyager data. It is shown that the increase of electron density in LISM (as compared with that obtained on the pulsar observations) gives rise to the coincidence of the model with the measurements. These conclusions do not contradict those of the Copernicus observations and the measurements of the scattered solar Lyman-alpha radiation.
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