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		题名	作者	年代	出处	被引量
	1	Electrochemical Luminescence-based Homogeneous Immunosensor显示文摘	TANAKA M KAMIYA S SHIBUE A	1993	Sensors and Actuators B1993，13，13：	1
	2	Metastatic colonization:settlement,adaptation and propagation of tumor cells in a foreign tissue environment显示文摘	SHIBUE T WEINBERG R A		0，，02：	1
	3	Quantitative description of soil organic matter dynamics-A review of approaches with reference to rice-based cropping systems 显示文摘	Shibu M E Leffelaar P A Keulen H V	2006	Geoderma2006，137，：	1
	4	Electrochemical luminescence based homogenous i mmunosensor显示文摘	Tanaka M Kamiya S Shibue A	1993	Sensors & Actuators B Chemicals1993，13，13：	1
	5	Targeting the Bcl-2 family for cancer therapy显示文摘	Shibu Thomas Bridget A Quinn Swadesh K Das Rupesh Dash Luni Emdad Santanu Dasgupta Xiang-Yang Wang Paul Dent John C Reed Maurizio Pellecchia Devanand Sarkar Paul B Fisher	2013	Expert Opinion on Therapeutic Targets2013，，1：	1
	6	Targeting the Bcl-2 family for cancer therapy 显示文摘	Shibu Thomas Bridget A Qui Swadesh K Das	2012	Expert Opinion on Therapeutic Targets2012，17，1：	1
	7	Targeting the Bcl-2 family for cancer therapy显示文摘	Shibu Thomas Bridget A Quinn Swadesh K Das Rupesh Dash Luni Emdad Santanu Dasgupta Xiang-Yang Wang Paul Dent John C Reed Maurizio Pellecchia Devanand Sarkar Paul B Fisher	2013	Expert Opinion on Therapeutic Targets2013，，1：	1
	8	On the line profile changes observed during the X2.2 class flare in the active region NOAA 11158显示文摘The solar active region NOAA 11158 produced a series of flares during its passage through the solar disk.The first major flare(of class X2.2) of the current solar cycle occurred in this active region on 2011 February 15 around 01:50 UT.We have analyzed the Dopplergrams and magnetograms obtained by the Helioseismic and Magnetic Imager(HMI) instrument onboard Solar Dynamics Observatory to examine the photospheric velocity and magnetic field changes associated with this flare.The HMI instrument provides high-quality Doppler and magnetic maps of the solar disk with 0.5 spatial scale at a cadence of 45 s along with imaging spectroscopy.We have identified five locations of velocity transients in the active region during the flare.These transient velocity signals are located in and around the flare ribbons as observed by Hinode in the Ca II H wavelength and the footpoints of hard X-ray enhancement are in the energy range 12–25 keV from RHESSI.The changes in shape and width of two circular polarization states have been observed at the time of transients in three out of five locations.Forward modeling of the line profiles shows that the change in atmospheric parameters such as magnetic field strength,Doppler velocity and source function could explain the observed changes in the line profiles with respect to the pre-flare condition.	Ankala Raja Bayanna Brajesh Kumar Parameswaran Venkatakrishnan Shibu Kunchandy Mathew Belur Ravindra Savita Mathur Rafael A Garcia	2014	Research in Astronomy and Astrophysics2014，14，2：	0

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