A method for reconstructing the solar-wind stream structure beyond Earth’s orbit

Abstract

The paper describes a new method for reconstructing the solar wind stream structure beyond Earth’s orbit. The method is based on the use of two-station interplanetary scintillation data obtained at decameter wavelengths. Solar wind stream structure is reconstructed by fitting model characteristics to the experimental ones. The model characteristics were obtained by using Feynman path-integral technique. Authors use multiflow model of the solar wind.