Statistics – Computation
Scientific paper
Apr 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986p%26ss...34..403k&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 34, April 1986, p. 403-408.
Statistics
Computation
Collisionless Plasmas, Computational Astrophysics, Ion Production Rates, Magnetohydrodynamic Flow, Time Dependence, Cometary Atmospheres, Conservation Equations, One Dimensional Flow, Solar Wind
Scientific paper
The flow of a magnetized llisionless plasma can to a large extent be treated in terms of hydrodynamics. If in addition to the plasma neutral particles are present which are added to the flow by some ionization process, a 'mass loading' of the plasma takes place. In this letter we investigate with the aid of an appropriate numerical code the time-dependent solutions of this problem in a one-dimensional geometry. Extensive computer experiments reveal that, depending on the initial conditions, there exists a variety of qualitatively different solutions. Only in certain cases the solutions approach a steady state.
Koemle Norbert I.
Lichtenegger Herbert I. M.
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