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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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  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

  S.V.Shestov, A.M.Urnov, S.V.Kuzin, I.A.Zhitnik, S.A.Bogachev,
Electron Density Diagnostics for Various Plasma Structures of the Solar Corona Based on Fe XI - Fe XIII Lines in the Range 176-207 A Measured in the SPIRIT/CORONAS-F Experiment Astronomy Letters, V. 35, No. 1, pp. 45-56, 2009
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  I.A.Zhitnik, S.V.Kuzin, A.M.Urnov, I.L.Beigman, S.A.Bozhenkov, I.Yu.Tolstikhina,
Extreme Vacuum Ultraviolet Solar Spectra Obtained during the SPIRIT Experiment aboard CORONAS-F: A Catalog of Lines in the Range 280–330 A Astronomy Letters, vol. 31, No. 1, pp. 37-56, 2005
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  S.V.Shestov, S.A.Bozhenkov, I.A.Zhitnik, S.V.Kuzin, A.M.Urnov, I.L.Beigman, F.F.Goryaev, I.Yu.Tolstikhina,
Solar EUV Spectra Obtained during the SPIRIT Experiment Onboard the CORONAS-F Satellite: A Catalog of Lines in the Range 176–207 A
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  A.M.Urnov, S.V.Shestov, S.A.Bogachev, F.F.Goryaev, I.A.Zhitnik, S.V.Kuzin,
On the Spatial and Temporal Characteristics and Formation Mechanisms of Soft X-ray Emission in the Solar Corona Astronomy Letters, vol. 33, No. 6, pp. 396-410
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  S.A.Bogachev, S.V.Kuzin, I.A.Zhitnik, A.M.Urnov, V.V.Grechnev,
" Dynamics of High-Temperature Plasma in the Solar Corona Using Spirit Observations in the MgXII 8.42 A line ". Solar System Research, Volume 39, Issue 6, pp.508-512, 2005.
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  I.A.Zhitnik, S.V.Kuzin, I.I.Sobelman, O.I.Bugaenko, A.P.Ignat'ev, A.V.Mitrofanov, S.N.Oparin, A.A.Pertsov, V.A.Slemzin, N.K.Suhodrev, A.M.Urnov,
" Main Results of the SPIRIT Experiment Onboard the CORONAS-F Satellite ". Solar System Research, Volume 39, Issue 6, pp.442-452, 2005.

  I.A.Zhitnik, S.V.Kuzin, A.M.Urnov, I.L.Beigman, S.A.Bozhenkov, I.Yu.Tolstikhina,
" Extreme vacuum ultraviolet solar spectra obtained during the SPIRIT experiment aboard CORONAS-F: A catalog of lines in the range 280 330 AA ". Astronomy Letters, vol. 31, Issue 1, p.37-56, 2005.