Collisionless deceleration model of the solar wind

Details Collisionless deceleration model of the solar wind Collisionless deceleration model of the solar wind

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ge%26ae..17..976g&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 17, Nov.-Dec. 1977, p. 976-983. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Collisionless Plasmas, Interstellar Gas, Solar Wind Velocity, Acoustic Velocity, Adiabatic Flow, Charge Exchange, Deceleration, Gas Density, Gas Dynamics, Gas Ionization, Gravitational Effects, Shock Wave Propagation

Scientific paper

The dynamics of the interstellar gas in the gravitational field of the sun is analyzed, treating the motion of the sun with respect to the gas as a hydrodynamic flow in the field of a point source. It is shown that deceleration of the interstellar gas in the solar gravitational field leads to a substantial increase in gas density. The influence of the charge-exchange between ions and (interstellar) hydrogen atoms on the deceleration of the solar wind is examined.

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