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.

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