Physics
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...232..556f&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 232, no. 2, June 1990, p. 556-564.
Physics
14
Heliosphere, Interstellar Gas, Ionization, Neutral Gases, Solar Radiation, Boltzmann Transport Equation, Density Distribution, Field Theory (Physics), Fourier Transformation, Integral Equations, Velocity Distribution
Scientific paper
A Fourier transformation, with respect to space and time coordinates, is done on the Boltzmann equation for the kinetic theory of neutral gases of the local interstellar medium when they are subject to solar force fields and ionization fields as they penetrate the inner heliosphere. Solutions are then generated for the Fourier-transformed velocity distribution function. By taking the space and time variabilities of the solar fields as known, the distribution function can be represented as an implicit function of the Fourier-transformed solar fields. An explicit solution is given for the Fourier-transformed neutral gas density, which can serve as a powerful means of interpreting very large numbers of interplanetary resonance glow data.
Fahr Hans Jörg
Scherer Klaus
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