Transport properties of high-temperature Jupiter atmosphere components

被引：64

作者：

Bruno, D. ^{[1
]}

Catalfamo, C. ^{[2
]}

Capitelli, M. ^{[1
,2
]}

Colonna, G. ^{[1
]}

De Pascale, O. ^{[1
]}

Diomede, P. ^{[2
]}

Gorse, C. ^{[1
,2
]}

Laricchiuta, A. ^{[1
]}

Longo, S. ^{[1
,2
]}

Giordano, D. ^{[3
]}

Pirani, F. ^{[4
]}

机构：

[1] Univ Bari, Dept Chem, I-70125 Bari, Italy

[2] CNR IMIP Bari, I-70125 Bari, Italy

[3] ESA ESTEC, Aerothermodynam Sect, NL-2200 AG Noordwijk, Netherlands

[4] Univ Perugia, Dept Chem, I-06123 Perugia, Italy

来源：

PHYSICS OF PLASMAS | 2010年 / 17卷 / 11期

关键词：

COLLISION INTEGRALS; ELASTIC-SCATTERING; CHARGE-TRANSFER; CROSS-SECTIONS; ELECTRON-SCATTERING; SLOW COLLISIONS; HYDROGEN; COEFFICIENTS; ENERGIES; HELIUM;

D O I：

10.1063/1.3495980

中图分类号：

O35 [流体力学]; O53 [等离子体物理学];

学科分类号：

070204 ; 080103 ; 080704 ;

摘要：

Transport properties of high-temperature helium and hydrogen plasmas as well as Jupiter atmosphere have been calculated for equilibrium and nonequilibrium conditions using higher approximations of the Chapman-Enskog method A complete database of transport cross sections for relevant interactions has been derived, including minority species, by using both ab initio and phenomenological potentials Inelastic collision integrals terms, due to resonant charge-exchange channels, have been also considered (C) 2010 American Institute of Physics [doi 10 1063/1 3495980]

引用

页数：16

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