Physics
Scientific paper
Dec 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990p%26ss...38.1487s&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 38, Dec. 1990, p. 1487-1493.
Physics
2
Heliosphere, Hydrogen, Interstellar Matter, Magnetohydrodynamic Turbulence, Boltzmann Transport Equation, Interplanetary Medium, Lyman Alpha Radiation, Shock Waves, Solar Radiation, Spatial Distribution
Scientific paper
The paper presents a theoretical approach describing the distribution function of the local-interstellar-medium (LISM) neutral hydrogen in the heliosphere and taking into account time-dependent solar and interstellar boundary conditions. The adequate Boltzmann-Vlasov differential equation is Fourier-transformed with respect to time and space coordinates, and then, instead of aiming at solutions for the hydrogen distribution function in configuration space coordinates, solutions of the Fourier-transformed distribution function are presented. Very general non-Maxwellian distribution functions are allowed along with time-dependent LISM boundary conditions to account for a case when some LISM turbulence patterns or nonlinear wavelike shock structures pass over the solar system.
Fahr Hans Jörg
Scherer Klaus
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