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Solar VUV telescope for nanosatellites
Russian version
DOI: 10.21883/TP.2022.13.52216.115-21
Kuzin S.V. 1,2, Bogachev S.A. 3,4, Erkhova N.F. 3, Pertsov A.A. 2,3,4, Loboda I.P. 3, Reva A.A. 3, Kholodilov A.V.3, Ulyanov A.S. 3, Kirichenko A.S. 2,3,4, Malyshev I.V.5,6, Pestov A.E. 5,6, Polkovnikov V.N. 5, Toropov M.N. 5,6, Tsybin N.N.5, Chkhalo N.I. 5, Kryukovskiy V.A.7, Gorev V.N.8, Doroshkin A.A.8, Zadorozhny A.M.8, Prokopyev V.Yu.8
1Shubnikov Institute of Crystallography “Crystallography and Photonics”, Russian Academy of Sciences, Moscow, Russia
2Institute Of Solar-Terrestrial Physics Of Siberian Branch Of Russian Academy Of Sciences (ISTP SB RAS), Irkutsk, Russia
3Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia
4Samara National Research University, Samara, Russia
5Institute for Physics of Microstructures, Russian Academy of Sciences, Nizhny Novgorod, Russia
6"Interoptics" ltd, Nizhny Novgorod, Russia
7Joint Company ‘Research and Production Corporation ‘Space Monitoring Systems, Information & Control and Electromechanical Complexes’ named after A.G. Iosifian’, Moscow, Russia
8Novosibirsk State University, Novosibirsk, Russia
Email: kirichenkoas@lebedev.ru
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Within the Universat program, a set of solar vacuum ultraviolet (VUV) telescopes has been developed for deployment on 6U nanosatellites. Telescopes are designed to get images of the solar corona. The spectral ranges of observations is considered, the characteristics of the nanosatellite from the point of view of the observations feasibility are opmized, the optical scheme of the telescope and VUV multilayer mirrors coatings and thin-film filters are modelled. Keywords: Nanosatellite, VUV, telescope, solar corona.
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