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				|  | S.Gburek,    										J.Sylwester,    										M.Kowalinski, SphinX Soft Xray Spectrophotometer: Science Objectives,
Design and Performance Solar System Research, 2011, Vol. 45, No. 3, pp. 189-199
 
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				|  | A.A.Reva,    										S.V.Shestov,    										S.A.Bogachev,    										S.V.Kuzin, Investigation of Hot X-Ray Points (HXPs) Using Spectroheliograph Mg XII Experiment Data from CORONAS-F/SPIRIT Solar Physics, V. 276, P. 97-112, 2012
 
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				|  | S.V.Kuzin,    										S.A.Bogachev,    										A.A.Pertsov,    										S.V.Shestov,    										A.A.Reva,    										A.S.Ul'yanov, EUV Observations of the Solar Corona
with Superhigh Spatial Resolution in the ARCA Project Bulletin of the Russian Academy of Sciences: Physics, 2011, Vol. 75, No. 1, pp. 87-90.
 
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				|  | S.V.Kuzin,    										S.V.Shestov,    										S.A.Bogachev,    										A.A.Pertsov,    										A.S.Ul'yanov,    										A.A.Reva, Processing Method of Images Obtained
during the TESIS/CORONASPHOTON Experiment Solar System Research, 2011, Vol. 45, No. 2, pp. 174-181
 
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				|  | S.V.Kuzin,    										I.A.Zhitnik,    										S.V.Shestov,    										S.A.Bogachev,    										O.I.Bugaenko,    										A.P.Ignat'ev,    										A.A.Pertsov,    										A.S.Ul'yanov,    										A.A.Reva,    										V.A.Slemzin,    										N.K.Suhodrev, The TESIS Experiment on the CORONASPHOTON Spacecraft Solar System Research, 2011, Vol. 45, No. 2, pp. 162-173
 
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				|  | Results of solar observations by the CORONAS-F payload Advances in Space Research, V. 47, P. 1538-1543, 2011
 
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				|  | P.V.Stoeva,    										A.D.Stoev,    										S.V.Kuzin, Whight light corona at different phases of the solar cycle Sun and Geosphere, V. 6, 1, 2011
 
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				|  | B.Sylwester,    										J.Sylwester,    										A.J.Engell,    										S.V.Kuzin, Physical Characteristics of AR 11024 Plasma Based on SphinX and XRT Data Cent. Eur. Astrophys. Bull., V. 35, 1, P. 171-180, 2011
 
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