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| 1 | Global absorption center map of the mafic minerals on the Moon as viewed by CE-1 IIM data显示文摘Determining the global distribution of minerals on the Moon has been an important goal of lunar science. Hyperspectral remote sensing is an important approach to acquiring minerals on the Moon on the global scale. The wavelength of the absorption band center is the key parameter for identifying minerals with reflectance spectra as well as remote sensing data. The global absorption center map of the mafic minerals of the Moon was produced for the first time with the Chang’E-1 IIM data. This map shows the global distribution of mafic minerals such as orthopyroxenes, clinopyroxenes, and olivine and even plagioclase feldspar of the Moon. The validation for some representative areas indicates that the global map is reliable and even more detailed than the results derived from Clementine-data. Moreover, our method is insensitive to the topography and viewing and illumination geometries. The global absorption band center map not only contributes to the lunar science research, but also has other implications to be further studied. Moreover, the preprocessing methods such as calibration and correction introduced in this study can be useful in other research with IIM data. | WU YunZhao 1,4* , ZHANG Xia 2 , YAN BoKun 3 , GAN FuPing 3 , TANG ZeSheng 4 , XU AoAo 4 , ZHENG YongChun 5 & ZOU YongLiao 5 1 School of Geographic and Oceanographic Sciences, Nanjing University, Nanjing 210093, China 2 Institute of Remote Sensing Applications, Chinese Academy of Sciences, Beijing 100101, China 3 Institute for Remote Sensing Method, China Aero Geophysical Survey and Remote Sensing Center for Land and Resources, Beijing 100083, China 4 Collaborative Research Laboratory on Lunar and Planetary Exploration, Macao University of Science and Technology, Taipa, Macao, China 5 National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China | 2010 | Science China(Physics,Mechanics & Astronomy)2010，53，12： | 11 |
| 2 | The role of MC1R gene in buffalo coat color显示文摘Melanocortin-1 receptor (MC1R) plays a major role in pigmentation in many species.To investigate if the MC1R gene is associated with coat color in water buffalo,the coding region of MC1R gene of 216 buffalo samples was sequenced,which included 49 black river buffalo (Murrah and Nili-Ravi),136 swamp buffalo (Dehong,Diandongnan,Dechang,Guizhou,and Xilin) with white and gray body,and 31 hybrid offspring of river buffalo Nili-Ravi (or Murrah) and swamp buffalo.Among the three variation sites found,SNP684 was synonymous,while SNP310 and SNP384 were nonsynonymous,leading to p.S104G and p.I128M changes,respectively.Only Individuals carrying homozygote EBR/EBR were black.The genotype and phenotype analysis of the hybrid offspring of black river buffalo and gray swamp buffalo further revealed that the river buffalo type allele EBR or the allele carrying the amino acid p.104S was important for the full function of MC1R.The in silico functional analysis showed that the amino acid substitutions p.G104S and p.M128I had significant impact on the function of MC1R.Above results indicate that the allele EBR or the allele carrying the amino acid p.104S was associated with the black coat color in buffalo. | MIAO YongWang1,2,WU GuiSheng3,WANG Lei2,LI DaLin4,TANG ShouKun5,LIANG JianPing2,MAO HuaMing2,LUO HuaiRong3 & ZHANG YaPing1,6 1 Laboratory for Conservation and Utilization of Bio-resource,Yunnan University,Kunming 650091,China 2 Faculty of Animal Science and Technology,Yunnan Agricultural University,Kunming 650201,China 3 Kunming Institute of Botany,Chinese Academy of Sciences,Kunming 650204,China 4 Yunnan Institute of Buffalo Science and Technology,Kunming 650021,China 5 Animal Husbandry and Veterinary Station of Luxi city,Luxi 678400,China 6 State Key Laboratory of Genetic Resources and Evolution,Kunming Institute of Zoology,Chinese Academy of Sciences,Kunming 650223,China | 2010 | Science China(Life Sciences)2010，53，2： | 8 |
| 3 | Taura syndrome virus from Venezuela is a new genetic variant显示文摘 | C0t 5 I Navarro S Tang KF | 2008 | Aquaculture2008，284，14： | 1 |
| 4 | Comparative proteomic analysis of plasma from bipolar depression and depressive disorder: identification of proteins associated with immune regulatory显示文摘 | Jin Chen (1) (2) (3) ChengLong Huang (2) (3) (5) YiRen Song (1) (2) (3) HaiYang Shi (1) (2) (3) Dong Wu (2) (3) (5) YongTao Yang (2) (3) (4) ChengLong Rao (2) (3) (7) Li Liao (2) (3) (5) You Wu (2) (3) (6) JianYong Tang (2) (3) (5) Ke Cheng (1) (2) (3) Jian Zhou (2) (3) Peng Xie (1) (2) (3) | 2015 | Protein & Cell2015，6，12： | 1 |
| 5 | An analysis of interplanetary sources of geomagnetic storm during November 7-8, 1998显示文摘We analyzed the properties of the solar wind appeared during November 7–8, 1998. Results show that the spaceship ACE spotted a shock (hereinafter referred to as the first shock) at 07:33 UT, November 7. The sheath appeared from the first shock to 22:00 UT November 7. A magnetic cloud-like (MCL) was observed during the period from 22:00 UT November 7 to 11:50 UT, November 8. Another shock was observed at 04:19 UT, November 8 (the second shock). It is apparent that the second shock has entered the rear part of the MCL (MCL_2), though the former part of the MCL (MCL_1) was not affected by the second shock. The main phase of the geomagnetic storm is split into three steps for the convenience of SYM-H index analysis. Step 1 covers the period from the sudden storm commence (SSC) at 08:15 UT, November 7 to the moment of 22:44 UT, November 7. Step 2 starts from 22:44 UT, November 7 and ends at 04:51 UT, November 8. The last step runs from 04:51 UT, November 8 to 06:21 UT, November 8. Step 2 has played a key role in the main development phase of the geomagnetic storm. Analysis of the solar wind properties associated with the main phase shows that the three steps in the main phase have sheath, MCL_1, and MCL_2 as their respective interplanetary source. Specifically, the sheath is covered by the solar wind data from 07:33 UT to 22:00 UT, November 7, MCL1 by the solar wind data from 22:00 UT, November 7 to 04:19 UT November 8, and MCL_2 by the solar wind data from 04:19 UT to 05:57 UT, November 8. MCL_1 had a strong and long lasting so UTh directed magnetic field, allowing it to play a key role in the development of the main phase. MCL_2 made a much smaller contribution to the main development phase, compared with MCL_1. | LE GuiMing1,2,3, TANG YuHua1, ZHENG Liang5 & LIU LianGuang4 1 Department of Astronomy, Nanjing University, Nanjing 210093, China 2 National Center for Space Weather, China Meteorological Administration, Beijing 100081, China 3 Key Laboratory of Radiometric Calibration and Validation for Environmental Satellites, China Meteorological Administration (LRCVES/CMA), Beijing 100081, China 4 North China Electric Power University, Beijing 102206, China 5 Graduate University of Chinese Academy of Sciences, Beijing 100049, China | 2010 | Chinese Science Bulletin2010，55，9： | 1 |
| 6 | New observations on atrial fibrillation before andafter surgical treatment in patients with the Wolff-Parkinson-White syndrome 显示文摘 | 5,Chen PS Pressley JC Tang ASL | 1992 | J AmColl Cardiol1992，19，： | 1 |
| 7 | Expression of intercellular adhesion molecule-1(ICAM-1)and vascular cell adhesion-1(VCAM-1)on proliferating vascular endothelial cellls in diahetil epiretinal members显示文摘 | Tang 5 le-Ruppert KC Gabel VP | 1994 | BrJOphthalmol1994，78，： | 1 |
| 8 | Thyroid hormone causes mitogen-activated protein kinase?dependent phosphorylation of the nuclear estrogen receptor显示文摘 | Tang HY Lin HY Zhang 5 | 2004 | Endocrinology2004，145，7： | 1 |
| 9 | EXPERIMENTAL STUDY ON CONTROLLING SEA WATER INTRUSIONBY FRESH WATER BARRIER显示文摘An experimental study on controlling sea water intrusion by fresh water barrier constructed bygroundwater recharge through ditch infiltration was carried out in the Laizhou gulf area of ShangdongProvince. By means of the physical and the numerical simulations and the field experiment, theempirical formulas for constructing fresh water barrier and the rule of its development, the controlscheme and the principle of its design as well as its application were preliminarily summarized. | LIU Qingyong1 DONG Guangqing2 GANG Shude3 WU Xiaofeng4 TANG Jie5 and LU Xianbi6(1,2,3 Shandong Provincial Institute of Water Resources, Jinan 250013, China.)(4,5,6 Department of Hydraulic and Hydropower Engineering, Tsinghua University, Beijing 100084 | 1999 | International Journal of Sediment Research1999，14，4： | 1 |
| 10 | Porous silica nanocapsules c self-assembly synthesis release显示文摘 | Chen H He J Tang H eta and nanopsheres: Dynam and application incontrolled 20(18): 5 894-5 900 | 2008 | Chem Mat2008，，： | 1 |
| 11 | Online weighted LS -SVM for hysteretie structural system identifieation 显示文摘 | Tang H 5 Xue 5 T Chen R | 2006 | Eng Struct2006，28，12： | 1 |
| 12 | Study of proton resonances in ^(18)Ne via resonant elastic scattering of ^(17)F+p and its astrophysical implication显示文摘The proton resonant properties in 18Ne, which determine the reaction rate of the key stellar 14O(α,p)17F reaction, have been studied by using a technique of proton resonant elastic scattering of 17F+p. A 4.22 MeV/nucleon 17F radioactive ion (RI) beam was produced via a projectile-fragmentation reaction, and separated by a Radioactive Ion Beam Line in Lanzhou (RIBLL). By bombarding a thick (CH2)n target, the energy spectra of the recoiled protons were measured by two ΔE-E silicon telescopes at the center-of-mass scattering angles of θc.m.≈175°±5°, θc.m.≈152°±8°, respectively. Several proton resonances in 18Ne were ob served clearly. A further R-matrix analysis of the experimental data is under way to determine the resonant parameters. The present work reports the preliminary results briefly. | HE JianJun1, HU Jun1,2, XU ShiWei1, CHEN ZhiQiang1, ZHANG XueYing1, WANG JianSong1, YU XiangQing1, ZHANG LiYong1,2, LI Long1,2, YANG YanYun1,2, MA Peng1,2, ZHANG XueHeng1, HU ZhengGuo1, GUO ZhongYan1, XU Xing1,2, YUAN XiaoHua1, LU Wan1,2, YU YuHong1, ZANG YongDong1,2, TANG ShuWen1,2, YE RuiPing1,2, CHEN JinDa1,2, JIN ShiLun1,2, DU ChengMing1,2, WANG ShiTao1,2, MA JunBing1,2, LIU LongXiang1,2, BAI Zhen1,2, LEI XiangGuo1, SUN ZhiYu1, ZHANG YuHu1, ZHOU XiaoHong1, XU HuShan1, SU Jun3, LI ErTao3, WANG HongWei4, TIAN WenDong4 & LI XiangQing5 1 Institute of Modern Physics (IMP), Chinese Academy of Sciences, Lanzhou 730000, China 2 Graduate University of Chinese Academy of Sciences, Beijing 100049, China 3 China Institute of Atomic Energy (CIAE), Beijing 102413, China 4 Shanghai Institute of Applied Physics (SINAP), Chinese Academy of Sciences, Shanghai 201800, China 5 School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China | 2011 | Science China(Physics,Mechanics & Astronomy)2011，54，S1： | 0 |
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