Thermodynamic properties for the magnetosheath plasma near the subsolar region
碩士 === 國立中央大學 === 太空科學研究所 === 86 === Total 14 magnetosheath crossing events observed by AMPTE/ IRMduring 1984 to 1985 are used to study the thermodynamic propertiesfor the magnetosheath plasma near the subsolar region. Empirical polytropic...
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ndltd-TW-086NCU000690052015-10-13T11:06:16Z http://ndltd.ncl.edu.tw/handle/63066631860118945746 Thermodynamic properties for the magnetosheath plasma near the subsolar region 向日區磁鞘電漿之熱力探討 Wang, Y.C. 王玉慶 碩士 國立中央大學 太空科學研究所 86 Total 14 magnetosheath crossing events observed by AMPTE/ IRMduring 1984 to 1985 are used to study the thermodynamic propertiesfor the magnetosheath plasma near the subsolar region. Empirical polytropic equations wih temperature anisotropy areobtained from the best-fit of observations.Comparisons with the CGL and double-polytropic models are alsodiscussed. The magnetosheath crossings are devided into fiveequal spatoal areas based on their perturbation characteristics.All regions are analyzed in order to find their thermodynamicproperties. From the Earth's bow shock to the magnetopause, it isfound that the thermodynamic state will gradually evolve from anon-Maxwellian to an isothermal state and then approach to an adiabatic state near the magnetopause. J.K.Chao 趙寄昆 1998 學位論文 ; thesis 1 zh-TW |
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碩士 === 國立中央大學 === 太空科學研究所 === 86 === Total 14 magnetosheath crossing events observed by AMPTE/
IRMduring 1984 to 1985 are used to study the thermodynamic
propertiesfor the magnetosheath plasma near the subsolar region.
Empirical polytropic equations wih temperature anisotropy
areobtained from the best-fit of observations.Comparisons with
the CGL and double-polytropic models are alsodiscussed. The
magnetosheath crossings are devided into fiveequal spatoal areas
based on their perturbation characteristics.All regions are
analyzed in order to find their thermodynamicproperties. From
the Earth's bow shock to the magnetopause, it isfound that the
thermodynamic state will gradually evolve from anon-Maxwellian
to an isothermal state and then approach to an adiabatic state
near the magnetopause.
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J.K.Chao |
author_facet |
J.K.Chao Wang, Y.C. 王玉慶 |
author |
Wang, Y.C. 王玉慶 |
spellingShingle |
Wang, Y.C. 王玉慶 Thermodynamic properties for the magnetosheath plasma near the subsolar region |
author_sort |
Wang, Y.C. |
title |
Thermodynamic properties for the magnetosheath plasma near the subsolar region |
title_short |
Thermodynamic properties for the magnetosheath plasma near the subsolar region |
title_full |
Thermodynamic properties for the magnetosheath plasma near the subsolar region |
title_fullStr |
Thermodynamic properties for the magnetosheath plasma near the subsolar region |
title_full_unstemmed |
Thermodynamic properties for the magnetosheath plasma near the subsolar region |
title_sort |
thermodynamic properties for the magnetosheath plasma near the subsolar region |
publishDate |
1998 |
url |
http://ndltd.ncl.edu.tw/handle/63066631860118945746 |
work_keys_str_mv |
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