博碩士論文 86227023 完整後設資料紀錄

DC 欄位 語言
DC.contributor太空科學研究所zh_TW
DC.creator崔春山zh_TW
DC.creatorChin-San Chuangen_US
dc.date.accessioned2000-7-4T07:39:07Z
dc.date.available2000-7-4T07:39:07Z
dc.date.issued2000
dc.identifier.urihttp://ir.lib.ncu.edu.tw:88/thesis/view_etd.asp?URN=86227023
dc.contributor.department太空科學研究所zh_TW
DC.description國立中央大學zh_TW
DC.descriptionNational Central Universityen_US
dc.description.abstractThe problem of the existence of intermediate shock (IS), this is an unsolved problem based on the observed data and theoretical model. In this thesis, we focus on the stability of the IS using the plasma simulation study. First, We calculate the upstream parameters for different IS by theoretical model, then we created four kinds of IS. Secondary, we simulate and analyze the stability of each kind of the IS in MHD code. The results show that all modes of the IS are stable except of the mode IS 2-3. The last part is to study the stability of the IS in hybrid code. We found that only IS 1-3 can be stable. We must have advanced theoretical model and much more space observed data to help our research ofen_US
DC.subject中速震波zh_TW
DC.subject磁性流體力學zh_TW
DC.subjectIntermediate Shocken_US
DC.subjectMagnetohydrodynamicen_US
DC.title中速震波穩定性之模擬研究zh_TW
dc.language.isozh-TWzh-TW
DC.type博碩士論文zh_TW
DC.typethesisen_US
DC.publisherNational Central Universityen_US

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