Search Results - "Urnov, A M"

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  1. 1

    Solar plasma temperature diagnostics in flares and active regions from spectral lines in the range 280–330 Å in the SPIRIT/CORONAS-F experiment by Shestov, S. V., Kuzin, S. V., Urnov, A. M., Ul’yanov, A. S., Bogachev, S. A.

    Published in Astronomy letters (2010)
    “…Plasma temperature diagnostics in solar flares and active regions has been carried out using data from the SPIRIT spectroheliograph onboard the CORONAS-F…”
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    Journal Article
  2. 2

    Electron density diagnostics for various plasma structures of the solar corona based on Fe XI-FeXIII lines in the range 176–207 Å measured in the SPIRIT/CORONAS-F experiment by Shestov, S. V., Urnov, A. M., Kuzin, S. V., Zhitnik, I. A., Bogachev, S. A.

    Published in Astronomy letters (2009)
    “…The relative intensities of FeXI-Fe XIII lines in the range 176–207 Å have been measured for various plasma structures of the solar corona using data from the…”
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    Journal Article
  3. 3

    On the spatial and temporal characteristics and formation mechanisms of soft X-ray emission in the solar corona by Urnov, A M, Shestov, S V, Bogachev, S A, Goryaev, F F, Zhitnik, I A, Kuzin, S V

    Published in Astronomy letters (01-06-2007)
    “…Our main goal is to show that the spatial and temporal dynamics of the temperature content for plasma structures in the solar corona can be described…”
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  4. 4

    Fe xii emission lines in solar active regions observed by the RES-C spectroheliograph on the CORONAS-I mission by Zhitnik, I. A., Kuzin, S. V., Urnov, A. M., Keenan, F. P., Pinfield, D. J.

    “…Theoretical line intensity ratios involving Fe xii transitions in the 186–201 Å wavelength range are compared with observational data for five solar active…”
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    Main Results of the SPIRIT Experiment Onboard the CORONAS-F Satellite by Zhithik, I A, Kuzin, S V, Sobel'man, I I, Bugaenko, O I, Ignat'ev, A P, Mitrofanov, A V, Oparin, S N, Pertsov, A A, Slemzin, V A, Sukhodrev, N K, Urnov, A M

    Published in Solar system research (01-11-2005)
    “…The main results of the SPIRIT experiment on imaging spectroscopy of the Sun in the soft X-ray and extreme vacuum UV range are presented. The results were…”
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    Physics of post-eruptive solar arcades: Interpretation of RATAN-600 and STEREO spacecraft observations by Livshits, M. A., Urnov, A. M., Goryaev, F. F., Kashapova, L. K., Grigor’eva, I. Yu, Kal’tman, T. I.

    Published in Astronomy reports (01-10-2011)
    “…Results of simultaneous measurements of radiation fluxes from post-eruption arcades on the Sun at 171, 195, 284, and 304 Å (from STEREO spacecraft data) and at…”
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    Journal Article
  9. 9

    Solar EUV spectra obtained during the SPIRIT experiment onboard the CORONAS-F satellite: A catalog of lines in the range 176–207 Å by Shestov, S. V., Bozhenkov, S. A., Zhitnik, I. A., Kuzin, S. V., Urnov, A. M., Beigman, I. L., Goryaev, F. F., Tolstikhina, I. Yu

    Published in Astronomy letters (2008)
    “…We present a catalog of 65 spectral lines in the range 176–207 Å recorded by the RES spectroheliograph in active regions and flares during the SPIRIT…”
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    Journal Article
  10. 10

    Atomic data for doubly-excited states 2lnl′ of He-like ions and 1s2lnl′ of Li-like ions with Z=6–36 and n=2,3 by Goryaev, F.F., Vainshtein, L.A., Urnov, A.M.

    Published in Atomic data and nuclear data tables (01-01-2017)
    “…The wavelengths and radiative transition probabilities for transitions 2lnl′→1snl″, 2lnl′→1s2l″, 1s2lnl′→1s2nl″, 1s2lnl′→1s22l″, and the autoionization decay…”
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  11. 11

    Dynamic 10 MK plasma structures observed in monochromatic full-Sun images by the SPIRIT spectroheliograph on the CORONAS-F mission by Zhitnik, I. A., Bugaenko, O. I., Ignat'ev, A. P., Krutov, V. V., Kuzin, S. V., Mitrofanov, A. V., Oparin, S. N., Pertsov, A. A., Slemzin, V. A., Stepanov, A. I., Urnov, A. M.

    “…High-resolution temporal series of monochromatic full-Sun images in the L Mg xii emission line at 8.42 Å have been obtained by the SPectroheliographIc X-Ray…”
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  12. 12

    Long-lived hot coronal structures observed with CORONAS-F/SPIRIT in the Mg XII line by Grechnev, V V, Kuzin, S V, Urnov, A M, Zhitnik, I A, Uralov, A M, Bogachev, S A, Livshits, M A, Bugaenko, O I, Zandanov, V G, Ignat'ev, A P, Krutov, V V, Oparin, S N, Pertsov, A A, Slemzin, V A, Chertok, I M, Stepanov, A I

    Published in Solar system research (01-07-2006)
    “…Large-scale hot features were detected and observed several times high in the solar corona in the high-temperature Mg XII line (T = 5-20 MK, T ^sub max^ = 10…”
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  13. 13

    X-ray and EUV diagnostics of active plasma structures with the RES spectroheliograph in the SPIRIT experiment onboard the CORONAS-F satellite by Zhitnik, I A, Kuzin, S V, Urnov, A M, Bogachev, S A, Goryaev, F F, Shestov, S V

    Published in Solar system research (01-07-2006)
    “…We provide a brief overview of the main methods and results of spectroscopic studies of several active plasma structures in the solar corona with the RES…”
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    Journal Article
  14. 14

    The Dynamics of High-Temperature Plasma in the Solar Corona according to SPIRIT Observations in Mg XII 8.42 Å Line by Bogachev, S. A., Kuzin, S. V., Zhitnik, I. A., Urnov, A. M., Grechnev, V. V.

    Published in Solar system research (01-11-2005)
    “…The spatial-distribution dynamics of the hot coronal plasma with T 10 MK during a period of high solar activity is studied. We analyze images of the NOAA 9830…”
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    On electron impact ionization cross-sections and rates for multiply charged ions by Shevelko, V. P., Urnov, A. M., Vainshtein, L. A., Müller, A.

    “…The electron impact ionization cross-sections σ and rates $\langle v\sigma\rangle$ for multiply charged ions are calculated using the Coulomb–Born…”
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    An iterative method in a probabilistic approach to the spectral inverse problem: Differential emission measure from line spectra and broadband data by Goryaev, F. F, Parenti, S, Urnov, A. M, Oparin, S. N, Hochedez, J. -F, Reale, F

    Published 25-10-2010
    “…A&A 523, A44 (2010), 15 pp Inverse problems are of great importance in astrophysics for deriving information about the physical characteristics of hot…”
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    Solar plasma temperature diagnostics in flares and active regions from spectral lines in the range 280-330 Aa in the SPIRIT/CORONAS-F experiment by Shestov, S V, Kuzin, S V, Urnov, A M, Ul'yanov, A S, Bogachev, S A

    Published in Astronomy letters (01-01-2010)
    “…Plasma temperature diagnostics in solar flares and active regions has been carried out using data from the SPIRIT spectroheliograph onboard the CORONAS-F…”
    Get full text
    Journal Article