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

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dc.contributor.author Kalinichenko, N.N
dc.contributor.author Olyak, M.R
dc.contributor.author Konovalenko, A.A
dc.contributor.author Brazhenko, A.I
dc.contributor.author Ivantishin, O.L
dc.contributor.author Lytvynenko, O.A
dc.contributor.author Bubnov, I.N
dc.contributor.author Yerin, S.N
dc.contributor.author Kuhai, N.V.
dc.contributor.author Romanchuk, O.I.
dc.date.accessioned 2019-05-29T06:35:37Z
dc.date.available 2019-05-29T06:35:37Z
dc.date.issued 2017
dc.identifier.citation 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 uk_UA
dc.identifier.uri http://hdl.handle.net/123456789/331
dc.description.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. uk_UA
dc.language.iso en uk_UA
dc.subject method for reconstructing uk_UA
dc.title A method for reconstructing the solar-wind stream structure beyond Earth’s orbit uk_UA
dc.type Article uk_UA
dc.subject.udc 378 uk_UA


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