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Zhurnal Tekhnicheskoi Fiziki, 2021 Volume 91, Issue 10, Pages 1441–1447 (Mi jtf4911)

This article is cited in 1 paper

XXV International Symposium on Nanophysics and Nanoelectronics, Nizhny Novgorod, March 9--12, 2021
Plasma

Solar VUV telescope for nanosatellites

S. V. Kuzinab, S. A. Bogachevcd, N. F. Erkhovac, A. A. Pertsovbcd, I. P. Lobodac, A. A. Revac, A. A. Kholodilovc, A. S. Ulyanovc, A. S. Kirichenkocde, I. V. Malyshevef, A. E. Pestovef, V. N. Polkovnikove, M. N. Toropovef, N. N. Tsybine, N. I. Chkhaloe, V. A. Kryukovskiyg, V. N. Gorevh, A. A. Doroshkinh, A. M. Zadorozhnyh, V. Yu. Prokopyevh

a Institute of Cristallography Russian Academy of Sciences, Moscow
b Institute of Solar-Terrestrial Physics, Siberian Branch of Russian Academy of Sciences, Irkutsk
c P. N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow
d Samara National Research University
e Institute for Physics of Microstructures, Russian Academy of Sciences, Nizhnii Novgorod
f "Interoptics", Nizhny Novgorod
g Research and Production Corporation "Space Monitoring Systems, Information & Control and Electromechanical Complexes" named after A. G. Iosifian, Moscow
h Novosibirsk State University

Abstract: 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.

Received: 21.04.2021
Revised: 21.04.2021
Accepted: 21.04.2021

DOI: 10.21883/JTF.2021.10.51355.115-21



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