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

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dc.contributor.authorKalinichenko, N.N
dc.contributor.authorOlyak, M.R
dc.contributor.authorKonovalenko, A.A
dc.contributor.authorBrazhenko, A.I
dc.contributor.authorIvantishin, O.L
dc.contributor.authorLytvynenko, O.A
dc.contributor.authorBubnov, I.N
dc.contributor.authorYerin, S.N
dc.contributor.authorKuhai, N.V.
dc.contributor.authorRomanchuk, O.I.
dc.date.accessioned2019-05-29T06:35:37Z
dc.date.available2019-05-29T06:35:37Z
dc.date.issued2017
dc.description.abstractThe 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.uk_UA
dc.identifier.citationA 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. 7-13uk_UA
dc.identifier.urihttps://repository.gnpu.edu.ua/handle/123456789/331
dc.language.isoenuk_UA
dc.subjectmethod for reconstructinguk_UA
dc.subject.udc378uk_UA
dc.titleA method for reconstructing the solar-wind stream structure beyond Earth’s orbituk_UA
dc.typeArticleuk_UA

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014.04 Середня освіта (Математика)