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Transport properties of high-temperature Jupiter atmosphere components
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10.1063/1.3495980
/content/aip/journal/pop/17/11/10.1063/1.3495980
http://aip.metastore.ingenta.com/content/aip/journal/pop/17/11/10.1063/1.3495980

## Figures

FIG. 1.

Viscosity of equilibrium helium plasma, at 1 atm pressure, compared with results by Capitelli (Ref. 63) (open circles) and by Aubreton (Ref. 5) (open triangles).

FIG. 2.

Total thermal conductivity of equilibrium helium plasma, at 1 atm pressure, compared with results by Capitelli (Ref. 63) (open circles) and by Aubreton (Ref. 5) (open triangles).

FIG. 3.

Viscosity of equilibrium hydrogen plasma, at 1 atm pressure, compared with results by different authors. Capitelli (Ref. 64) (dotted line), Devoto (Ref. 65) (closed squares), Murphy (Ref. 6) (open circles), and Boulos (Ref. 66) (open triangles).

FIG. 4.

Total thermal conductivity of equilibrium hydrogen plasma, at 1 atm pressure, compared with results by different authors. Capitelli (Ref. 64) (dotted line), Devoto (Ref. 65) (closed squares), Murphy (Ref. 6) (open circles), and Boulos (Ref. 66) (open triangles).

FIG. 5.

Viscosity for single species (lines) compared with results by Biolsi (Ref. 1) (open markers) and by Hansen (Ref. 2) (closed markers).

FIG. 6.

Viscosity of equilibrium Jupiter atmosphere, at 1 atm pressure, compared with results by Biolsi (Ref. 1) (open circles) and by Hansen (Ref. 2) (open triangles).

FIG. 7.

Total thermal conductivity of equilibrium Jupiter atmosphere, at 1 atm pressure, compared with results by Biolsi (Ref. 1) (open circles) and by Hansen (Ref. 2) (open triangles).

FIG. 8.

Internal thermal conductivity of equilibrium Jupiter atmosphere, at 1 atm pressure, compared with results by Biolsi (Ref. 1) (open circles). The results obtained by Bruno (Ref. 70) for equilibrium hydrogen plasma including (dash-dotted line) and neglecting (dotted line) the effect of electronically excited states are also reported.

FIG. 9.

Viscosity as a function of temperature for strongly nonequilibrium conditions of Jupiter atmosphere, at 1 atm pressure, compared with equilibrium case (see Table X for fixed compositions).

FIG. 10.

Partial translational thermal conductivity as a function of temperature for strongly non-equilibrium conditions of Jupiter atmosphere, at 1 atm pressure, compared with equilibrium case.

FIG. 11.

Electrical conductivity as a function of temperature for strongly nonequilibrium conditions of Jupiter atmosphere, at 1 atm pressure, compared with equilibrium case.

## Tables

Table I.

Fitting coefficients, entering Eq. (11), for in heavy-particle interactions.

Table II.

Polarizability values for Jupiter atmosphere species.

Table III.

Fitting coefficients, entering Eq. (11), for in -neutral interactions.

Table IV.

Parameters of phenomenological potential for interactions relevant to Jupiter atmosphere.

Table V.

Fitting coefficients, entering Eq. (17), for in neutral-ion interactions [to be added to the elastic contribution in order to obtain the effective odd-order collision integrals by Eq. (16)].

Table VI.

Fitting coefficients, entering Eq. (19), for in electron-neutral interactions.

Table VII.

Transport coefficients {viscosity [kg/(m s)], electrical conductivity (S/m), thermal conductivity contributions [W/(m K)]} of equilibrium helium plasma.

Table VIII.

Transport coefficients {viscosity [kg/(m s)], electrical conductivity (S/m), thermal conductivity contributions [W/(m K)]} of equilibrium hydrogen plasma.

Table IX.

Transport coefficients {viscosity [kg/(m s)], electrical conductivity (S/m), and thermal conductivity contributions [W/(m K)]} of equilibrium ten-species Jupiter atmosphere.

Table X.

Nonequilibrium compositions, cases .

/content/aip/journal/pop/17/11/10.1063/1.3495980
2010-11-19
2014-04-18

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