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

页码：613 / 621

页数：9

共 36 条

[1]

[Anonymous], 1973, WILEY SERIES PLASMA

[2]

[Anonymous], 1953, The Mathematical Theory of Non-Uniform Gases

[3]

[Anonymous], 1964, Molecular theory of gases and liquids

[4] SEMICLASSICAL CALCULATIONS OF TRANSPORT-COEFFICIENTS AND ROTATIONAL RELAXATION OF NITROGEN AT HIGH-TEMPERATURES [J].