Computer Science
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esast.246.....c&link_type=abstract
Tables of internal partition functions and thermodynamic properties of high-temperature Mars-atmosphere species from 50K to 5000
Computer Science
Mars Atmosphere: Components, Thermodynamic Properties
Scientific paper
High-temperature thermodynamic properties for Mars-atmosphere components (Ar, Ar+, Ar2+, Ar3+, Ar4+, C, C+, C2+, C3+, C4+, C-, C2, C2+, C2-, C3, CN, CN+, CN-, CO, CO+, CO2, CO2+, e-, N, N+, N2+, N3+, N4+, N-, N2, N2+, N2-, N3, NO, NO+, NO2, N2O, N2O+, CNO, O, O+, O2+, O3+, O4+, O-, O2, O2+, O2-, O3, O3-, C2N, C2O, CO2-) are presented and discussed. The present report is divided into two parts: in the first one, theoretical aspects of the calculation are described. Results are discussed and compared with previous works including aspects such as quasi-bound rotational states for molecules and cut-off criteria and autoionasing states for atomic species. The second part provides tables of spectroscopic data used in the calculation and thermodynamic properties in the temperature range from 50K to 50000K at P=1 bar. Finally, fitting coefficients for nondimensional specific heat are included.
Capitelli Mario
Casavola Alessandro
Colonna G.
Giordano Daniele
Marraffa Lionel
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