High temperature Mars atmosphere. Part II: transport properties

被引：24
作者：
Catalfamo, C. [1 ]
Bruno, D. [2 ]
Colonna, G. [2 ]
Laricchiuta, A. [2 ]
Capitelli, M. [1 ,2 ]
机构：
[1] CNR IMIP, Bari, Italy
[2] Univ Bari, Dept Chem, I-70100 Bari, Italy
来源：
EUROPEAN PHYSICAL JOURNAL D | 2009年 / 54卷 / 03期
关键词：
IONIZED MONATOMIC GASES; EQUILIBRIUM CALCULATION; COLLISION INTEGRALS; AIR PLASMAS; COEFFICIENTS; NITROGEN; MIXTURE;
D O I：
10.1140/epjd/e2009-00193-6
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
Transport coefficients of equilibrium Martian atmosphere have been calculated in the second non-vanishing Chapman-Enskog approximation and compared with existing literature results. The present work improves previous calculations by considering a very detailed chemistry model of Martian atmosphere that includes 53 species and by extending the temperature range up to 50 000 K.
引用
收藏
页码：613 / 621
页数：9
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