International Center for Astronomical, Medical and Ecological Research
     
 Observation and modeling of selected manganese lines in solar spectrum


Figure 1. The average over solar disk spectrum near the Mn I 543.2 nm spectral line (a) and the Mn I 543.2 nm spectral line profiles for different heliocentric angles (b)








Figures 2. Center-to-limb variation of the observed and calculated (circles - with hyperfine components, squares - without hyperfine components) parameters of the Mn I 543.2 nm spectral line




Telescopes Instrumentation
 2m RCC Telescope produced by Carl Zeiss Jena GmbH (Germany)
 Large Horizontal Solar Telescope  
 Zeiss-600 Telescope
 80-cm Telescope
 Small Solar Telescope SEF
 MAESTRO -
 MAtrix Echelle SpecTROgraph
 MMCS -
 Multi Mode Cassegrain
Spectrometer
 TUVES-
 Terskol Ultra Violet Echelle Spectrometer
 High-Speed Two-Channel Stellar Photometer
Activities80-cm Telescope
 Spectral investigations of interstellar clouds, solar analogs, X-ray binary stars, etc.
 Orbit calculation and monitoring of geosynchronous satellites
 Observation and modeling of selected manganese lines in solar spectrum
 Simultaneous observations with the Synchronous Network of Optical Telescopes to study microvariability of stars
  Study of gas and dust in comets
 Photometry and astrometry of the inner satellites of Jupiter and Saturn
 Atmospheric studies

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