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		题名	作者	年代	出处	被引量
	1	Optimisation of the two-dimensional gel electrophoresis protocol using the Taguchi approach显示文摘	Guennadi A K Iain M P Julian B J	2004	Proteome Science2004，，2：	1
	2	STJD14091800000193显示文摘	Oleg Shcherbakov Andrei Donets Alexander Evdokimov Alexander Fomichev Tokio Fukahori Akira Hasegawa Alexander Laptev Vladimir Maslov Guennady Petrov Sergei Soloviev Yuri Tuboltsev Alexander Vorobyev	2002	Journal of Nuclear Science and Technology (sup)2002，，2：	1
	3	Geometric Accuracy oflkonos:Zoom In 显示文摘	Guennadi A Guienko	2004	IEEE TRANSACTION ON GEOSCIENCE AND REMOTE SENSING2004，42，1：	1
	4	Intrathyroidal parathyroidglands:Small,but mighty(a Napoleonphenomenon)显示文摘	Haggi M Guennadi K David F	2012	Sui-ery2012，152，6：	1
	5	REAL-TIME OPTICAL MONITORING OF CAPILLARY GRID SPATIAL PATTERN IN EPITHELIUM BY SPATIALLY RESOLVED DIFFUSE REFLECTANCE PROBE显示文摘We developed a novel method for real-time monitoring of alteration of the local epithelium vessel/capillary and blood oxygenation spatial pattern in epithelium exploiting a compact fibre sensor system based on spatially and spectrally resolved diffuse reflectance.The method is based on collection of spatially resolved diffuse reflectance Re(λ)by fiber sensors.The spatial resolution is provided as a dependence of Re(λ)on a set of distancesρbetween the source and detector(attenuation curve).It is expected that the new method can reasonably extract the minor spatial deviations of oxygenation and local blood volume fraction-parameters,directly related to the local vessel density and capillary spatial patterns in the epithelium.Light scattering in visible range is naturally taken into account in the proposed method.	GUENNADI SAIKO ALEXANDRE DOUPLIK	2012	Journal of Innovative Optical Health Sciences2012，5，2：	0
	6	The importance of source positions during radio fine structure observations显示文摘The measurement of positions and sizes of radio sources in the observations of the fine structure of solar radio bursts is a determining factor for the selection of the radio emission mechanism. The identical parameters describing the radio sources for zebra structures(ZSs) and fiber bursts confirm there is a common mechanism for both structures. It is very important to measure the size of the source in the corona to determine if it is distributed along the height or if it is point-like. In both models of ZSs(the double plasma resonance(DPR) and the whistler model) the source must be distributed along the height, but by contrast to the stationary source in the DPR model, in the whistler model the source should be moving. Moreover, the direction of the space drift of the radio source must correlate with the frequency drift of stripes in the dynamic spectrum. Some models of ZSs require a local source, for example,the models based on the Bernstein modes, or on explosive instability. The selection of the radio emission mechanism for fast broadband pulsations with millisecond duration also depends on the parameters of their radio sources.	Guennadi P.Chernov Yi-Hua Yan Qi-Jun Fu	2014	Research in Astronomy and Astrophysics2014，14，7：	0

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