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Electron heat conduction under non-Maxwellian distribution in hohlraum simulation
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10.1063/1.3677357
/content/aip/journal/pop/19/1/10.1063/1.3677357
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/1/10.1063/1.3677357
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

(Color online) The coefficients , Cn , and as functions of the exponent m.

Image of FIG. 2.
FIG. 2.

(Color online) The 1-D spatial profiles of electron temperature at 1.0 ns obtained by using the NM model and the FL model with , , and , respectively.

Image of FIG. 3.
FIG. 3.

(Color online) The 1-D spatial profiles of electron number density and index m at 1.0 ns obtained by using the NM model.

Image of FIG. 4.
FIG. 4.

(Color online) The spatial distribution of the total flux and flux associated with the gradients of , , and index m at 1.0 ns obtained under the NM model. The spikes on the curve are due to the numerical fluctuations.

Image of FIG. 5.
FIG. 5.

(Color online) The spatial distributions of corresponding , Cn , and at 1.0 ns under the NM model.

Image of FIG. 6.
FIG. 6.

(Color online) The spatial distributions of the scale lengths of , ne , and m at 1.0 ns obtained under the NM model. The spikes on the curve are due to the numerical fluctuations.

Image of FIG. 7.
FIG. 7.

(Color online) The heat flux functions , , and for a non-Maxwellian distribution with versus .

Image of FIG. 8.
FIG. 8.

(Color online) The 1-D spatial profiles of at 1.0 ns obtained by using the NM model and FL model with flux limiters 0.05, 0.15, and 1.0.

Image of FIG. 9.
FIG. 9.

(Color online) The 1-D spatial distributions of line-emission at 1.0 ns obtained by using the NM model and FL model with flux limiters 0.05, 0.15, and 1.0.

Image of FIG. 10.
FIG. 10.

(Color online) The maps of in a quarter of hohlraum at 0.5 ns (a) and 1 ns (b) under the NM model and the FL model with 0.05, 0.15, and 1.

Image of FIG. 11.
FIG. 11.

(Color online) The radial distributions of at 1 ns at the axial position Z = 0.4 mm under the NM model and the FL model with of 0.05, 0.15, and 1.

Image of FIG. 12.
FIG. 12.

(Color online) The axial distributions of at 1 ns at the radial position mm under the NM model and the FL model at of 0.05, 0.15, and 1.

Image of FIG. 13.
FIG. 13.

(Color online) The radial distributions of at 1 ns at the axial position mm under the NM model and the FL model at of 0.05, 0.15, and 1.

Image of FIG. 14.
FIG. 14.

(Color online) The radial distributions of at 1 ns at the axial position mm under the NM model and the FL model with 0.05, 0.15, and 1.

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/content/aip/journal/pop/19/1/10.1063/1.3677357
2012-01-26
2014-04-19
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Electron heat conduction under non-Maxwellian distribution in hohlraum simulation
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/1/10.1063/1.3677357
10.1063/1.3677357
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