Stationary and supersonic proton fluxes parallel to the magnetic field

Details Stationary and supersonic proton fluxes parallel to the magnetic field Stationary and supersonic proton fluxes parallel to the magnetic field

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974cajph..52.2402f&link_type=abstract

Canadian Journal of Physics, vol. 52, Dec. 1, 1974, p. 2402-2421. In French.

Physics

Proton Flux Density, Solar Atmosphere, Solar Protons, Supersonic Flow, Transport Properties, Distribution Functions, Lines Of Force, Maxwell-Boltzmann Density Function, Partial Differential Equations, Solar Magnetic Field

Scientific paper

Using the gyration radius as the parameter to expand the differential equation for the moments, transport equations are obtained for highly supersonic flux parallel to the magnetic field. The maximum order one can hope to obtain for the invariants is discussed together with the relation between the function of distribution f-I proposed by Whang and that which must result at 1 AU if f-I or a bimaxwellian function are used at the origin.

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