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Laboratory of X-ray Astronomy of the Sun





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Solar Space Experiments in LPI

TESIS team

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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. 189Ц199
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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

 
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. 87Ц90.
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Processing Method of Images Obtained during the TESIS/CORONASPHOTON Experiment Solar System Research, 2011, Vol. 45, No. 2, pp. 174Ц181
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The TESIS Experiment on the CORONASPHOTON Spacecraft Solar System Research, 2011, Vol. 45, No. 2, pp. 162Ц173
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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. 797Ц807
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