Publications
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Wave-like Formation of Hot Loop Arcades |
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INITIATION AND EARLY EVOLUTION OF THE CORONAL MASS EJECTION ON MAY 13, 2009 FROM EUV AND WHITE-LIGHT OBSERVATIONS |
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SphinX Soft Xray Spectrophotometer: Science Objectives, Design and Performance Solar System Research, 2011, Vol. 45, No. 3, pp. 189–199 |
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S.V.Shestov, A.A.Reva, S.V.Kuzin, Extreme Ultraviolet Spectra of Solar Flares From the Extreme Ultraviolet Spectroheliograph SPIRIT onboard the CORONAS-F Satellite The Astrophysical Journal, V. 780, P. 15-31, 2014 |
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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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V.A.Slemzin, L.Harra, A.M.Urnov, S.V.Kuzin, F.F.Goryaev, D.Berghmans, Signatures of Slow Solar Wind Streamers from Active Regions in the Inner Corona Solar Physics, Volume 286, Issue 1, pp.157-184 |
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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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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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The TESIS Experiment on the CORONASPHOTON Spacecraft Solar System Research, 2011, Vol. 45, No. 2, pp. 162–173 |
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A.S.Kirichenko, S.A.Bogachev, Long-duration plasma heating in solar microflares of X-ray class A1.0 and lower Astronomy Letters, 2013, Vol. 39, No. 11, pp. 797–807 |
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