A method for reconstructing the solar-wind stream structure beyond Earth’s orbit
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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.
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A method for reconstructing the solar-wind stream structure beyond Earth’s orbit / Kalinichenko N.N., Olyak M.R., Konovalenko A.A., Brazhenko A.I., Ivantishin O.L., Lytvynenko O.A., Bubnov I.N., Yerin S.N., Kuhai N.V. , Romanchuk O.I. // Proceedings of the 9th Workshop "Solar influence on the magnetosphere, ionosphere and atmosphere". (Sunny beach, Bulgaria, 30 May – 3 June, 2017). p. 7-13