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dc.contributor.author Chubey, M.S.
dc.contributor.author Grigoriev, V.M.
dc.contributor.author Eroshkin, G.I.
dc.contributor.author L'vov, V.N.
dc.contributor.author Papushev, P.G.
dc.contributor.author Yagudin, L.I.
dc.date.accessioned 2015-04-03T16:49:03Z
dc.date.available 2015-04-03T16:49:03Z
dc.date.issued 2005
dc.identifier.citation Stereoscopic principle in space observatory / M.S. Chubey, V.M. Grigoriev, G.I. Eroshkin, V.N. L'vov, P.G. Papushev, L.I. Yagudin // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 172-175. — Бібліогр.: 8 назв. — англ. uk_UA
dc.identifier.issn 0233-7665
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/79636
dc.description.abstract The scientific team (ST) of the Interplanetary Solar Stereoscopic Observatory (ISSO) has got the financial support to finalize the scientific determination study with the aim to investigate the full potential of the stereoscopic idea and technical possibilities to realize the space stereoscope. The stereoscopic principle will work with optimal effectiveness in space under conditions of the stable stereoscopic base during the whole time interval of the experiment. The main conclusion of the ST up to now is that the ISSO may be created as the observatory with the flexible program, being able to support the extended solar physics investigations and the star investigations for stellar astronomy and astrophysics, being especially effective in the 3D astrometric monitoring of the motion of Solar System bodies, including near-Earth asteroids. uk_UA
dc.language.iso en uk_UA
dc.publisher Головна астрономічна обсерваторія НАН України uk_UA
dc.relation.ispartof Кинематика и физика небесных тел
dc.subject MS2: Physics of Solar Atmosphere uk_UA
dc.title Stereoscopic principle in space observatory uk_UA
dc.type Article uk_UA
dc.status published earlier uk_UA


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