Computer Science
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.533..111s&link_type=abstract
In: Proceedings of the First International Workshop on Radiation of High Temperature Gases in Atmospheric Entry, 8-10 October 20
Computer Science
Space Vehicles, Planetary Atmospheres, Entry
Scientific paper
A brief description is presented for a computing system (CS) MONSTER ("Monitor System for Transfer of Electromagnetic Radiation"), intended for numerical simulation of radiative gas dynamic problems and for creation of spectral optical models of hot gases and plasmas for aerospace application. The optical models can be created for temperatures T = 300-20,000K or T = 20,000-120,000K, for pressures p up to 1000 atm and for wavenumbers at the range 1000-500,000 cm-1. At present the CS MONSTER is provided with spectroscopic information and numerical simulation models for gas and plasma mixtures containing the following chemical elements: H, He, C, N, O, Si, Ar, Na, Mg, Al, K, Ca. Examples of different kinds of optical models are presented.
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