Mathematics
Scientific paper
Oct 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ge%26ae..14..784r&link_type=abstract
(Geomagnetizm i Aeronomiia, vol. 14, Sept.-Oct. 1974, p. 784-787.) Geomagnetism and Aeronomy, vol. 14, no. 5, 1974, p. 671-674.
Mathematics
Particle Flux Density, Radiation Pressure, Shock Wave Propagation, Solar Corpuscular Radiation, Solar Wind, Differential Equations, Ideal Gas, Magnetohydrodynamic Flow, Magnetohydrodynamic Stability, Mathematical Models, Solar Flares, Velocity Distribution, Zero Angle Of Attack
Scientific paper
Expressions are derived for the pressure and half-angle of a conical flux as functions of the velocity and half-angle of the shock wave. The steady motion of a cone in a homogeneous plasma with a uniform magnetic field is investigated. The cone axis, the intensity vector of the undisturbed magnetic field, and the plasma velocity vector in the coordinate system connected to the cone are assumed to be parallel. A domain of the parameters of motion is defined where stable flow is possible, and the minimum average energy of flow particles is estimated. The evaluations indicate that the available experimental data for any flow of energetic solar particles in the near earth space are insufficient for defining the shape of the flow.
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