磁化電漿中的尾波場

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DC Field	Value	Language
dc.contributor.author	張研俞	en_US
dc.contributor.author	Yen - Yu, Chang	en_US
dc.contributor.author	林貴林	en_US
dc.contributor.author	Lin- Guey, Lin	en_US
dc.date.accessioned	2014-12-12T01:17:29Z	-
dc.date.available	2014-12-12T01:17:29Z	-
dc.date.issued	2007	en_US
dc.identifier.uri	http://140.113.39.130/cdrfb3/record/nctu/#GT009527525	en_US
dc.identifier.uri	http://hdl.handle.net/11536/39022	-
dc.description.abstract	高能宇宙射線(UHECR)的來源，一直是天文物理所要探討的題目之一。其中利用太空中的電漿所產生之電場（尾波場），讓帶電粒子加速至極高能量，是可能的來源之一。本篇論文主要呈現利用數值分析的方法，探討在均勻磁場下之電漿，受到強場電磁波激發後，所產生之尾波場的行為。	zh_TW
dc.description.abstract	The source of ultra high energy cosmic ray (UHECR) has been a mystery in astrophysics for years. It has been proposed that the plasma wakefield acceleration could be a possible acceleration mechanism for UHECR. In this thesis, we present a numerical calculation of wakefield in the magnetized plasma, taking into account the relativistic effects.	en_US
dc.language.iso	en_US	en_US
dc.subject	電漿	zh_TW
dc.subject	電漿加速	zh_TW
dc.subject	尾波場	zh_TW
dc.subject	天文粒子	zh_TW
dc.subject	plasma	en_US
dc.subject	plasma acceleration	en_US
dc.subject	wakefield	en_US
dc.subject	UHECR	en_US
dc.title	磁化電漿中的尾波場	zh_TW
dc.title	Wakefield In Magnetized Plasma	en_US
dc.type	Thesis	en_US
dc.contributor.department	物理研究所	zh_TW
Appears in Collections:	Thesis

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