Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..331k&link_type=abstract
In ESA, Plasma Astrophysics p 331-334 (SEE N91-15046 06-90)
Astronomy and Astrophysics
Astrophysics
Constitutive Equations, Flow Distribution, Magnetic Fields, Magnetic Flux, Solar Wind, Azimuth, Current Sheets, Density Distribution, Earth Orbital Environments, Heliosphere, Mathematical Models, Statistical Distributions
Scientific paper
Using numerical calculations of Solar Wind (SW) flow, a study is made of the influence of the azimuthal distribution of its parameters near the Sun upon the SW structure in the space up to the Earth's orbit. It is shown that both the character and intensity of the interaction of fast and slow SW streams in interplanetary space and plasma properties in the region of the heliosphere current sheet which is carried away by the slow SW flow from the Sun to the Earth, depend on solar wind properties at small distances from the Sun and, in particular, on the character of the mass density and magnetic field distribution there.
Fainshtein V.. G.
Kaigorodov A. P.
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