Abstract
A method for the numerical solution of the non-stationary two-dimensional problem of the propagation relative to a moving interplanetary medium of a perturbation caused by the emission of finite energy within the limits of a section of a cone, simulating the chromospheric region of the sun occupied by the flare is discussed. The effect of solar gravitation and of the radial component of the magnetic field strength on the motion of the gas is taken into account.
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