One-dimensional kinematics of particle stream flow with application to solar wind simulation

Details One-dimensional kinematics of particle stream flow with application to solar wind simulation One-dimensional kinematics of particle stream flow with application to solar wind simulation

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985p%26ss...33..831o&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 33, July 1985, p. 831-839.

Mathematics

14

One Dimensional Flow, Particle Motion, Solar Wind Velocity, Velocity Distribution, Atmospheric Models, Spatial Distribution

Scientific paper

A simple kinematic method for determining the particle velocity distribution of a model solar wind for which the spatial distribution of particles is given as a function of particle travel time has been developed by Hakamada and Akasofu (1982). In this paper the authors formalize their method mathematically and derive an inverse procedure for determining the particle distribution from a given velocity distribution. This inverse procedure is then applied to a simulated velocity distribution obtained from an MHD finite difference code.

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