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 (303). 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.
The work is partially supported by RFBR (Grants 05-01-00682 and 05-02-16343).
Mathematical modelling in actual problems of science and technics