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6篇 您的检索式：作者名="Zschornack"

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		题名	作者	年代	出处	被引量
	1	Geometrical aberrations in curved bragg crystal spectrometer显示文摘	ZSCHORNACK G MULLER G MUSIOL G	1982	Nuclear Instruments and Methods1982，200，：	1
	2	Yield-scaled greenhouse gas emissions from flood irrigated rice under long-term conventional tillage and no-till systems in a Humid Subtropical climate显示文摘	Cimélio Bayer Falberni de Souza Costa Gabriel Munhoz Pedroso Tiago Zschornack Estefania S. Camargo Magda Aparecida de Lima Rosa T.S. Frigheto Juliana Gomes Elio Marcolin Vera Regina Mussoi Macedo	2014	Field Crops Research2014，，：	1
	3	Applying neural networks to performance estimation of embedded software 显示文摘	Oyamada M S Zschornack F Wagner F R	2008	Systems Architecture2008，54，1：	1
	4	First Results of Ion Trapping in the Dresden EBIT II显示文摘	U. Kentsch G. Zschornack F. Grossmann V. P. Ovsyannikov F. Ullmann	2003	Hyperfine Interactions (-)2003，，1：	1
	5	Production of highly charged argon ions from a room temperature electron beam ion trap显示文摘In this work, highly charged ions have been extracted from the advanced Electron Beam Ion Source(EBIS-A)developed in a scientific cooperation between the Dresden University of Technology and the DREEBIT GmbH Dresden.The charge state distributions of ions extracted from the EBIS-A are measured in the pulse and leaky modes under different operation conditions. Ar^(16+)ions with current of 2pA are produced and extracted in the leaky mode. 3×10~5 Ar^(18+)ions per pulse are extracted in the pulse mode.The ion charge state distribution is a function of the ionization time.	王铁山彭海波 Ovsyannikov V P Kentsch U Ullmann F 程锐 Zschornack G	2008	Chinese Physics C2008，32，5：	0
	6	A small electron beam ion trap/source facility for electron/neutral-ion collisional spectroscopy in astrophysical plasmas显示文摘Spectra are fundamental observation data used for astronomical research,but understanding them strongly depends on theoretical models with many fundamental parameters from theoretical calculations.Different models give different insights for understanding a specific object.Hence,laboratory benchmarks for these theoretical models become necessary.An electron beam ion trap is an ideal facility for spectroscopic benchmarks due to its similar conditions of electron density and temperature compared to astrophysical plasmas in stellar coronae,supernova remnants and so on.In this paper,we will describe the performance of a small electron beam ion trap/source facility installed at National Astronomical Observatories,Chinese Academy of Sciences.We present some preliminary experimental results on X-ray emission,ion production,the ionization process of trapped ions as well as the effects of charge exchange on the ionization.	Gui-Yun Liang Hui-Gang Wei Da-Wei Yuan Fei-Lu Wang Ji-Min Peng Jia-Yong Zhong Xiao-Long Zhu Mike Schmidt Günter Zschornack Xin-Wen Ma Gang Zhao	2018	Research in Astronomy and Astrophysics2018，18，1：	0

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