Modelling of the emission spectra of tungsten plasma

The calculations of tungsten emission spectra were carried out in a wide range of temperature and density ($30<T<150$ eV, $0.01<\rho<0.03$ g/cm$^3$). The calculated spectra may be usefull in the investigation of powerful wire arrays liners in TRINITI on Angara 5-1 and in Sandia on Z machine (USA) facilities. The code THERMOS & BELINE were used for computation of nonLTE spectra of plane and cylindrical tungsten layers. At most important cases the calculations were verified as for line position and also for more realistic geometry.