DEDICATED PRINCIPAL PROPERTIES FOR PEPTIDE QSARS: THEORY AND APPLICATIONS     

BERTSKAGERBERG  MICHAEL  SVANTEWOLD 《地理学报(英文版)》1990,(3)

  相似文献   

Oxide Mineralogy and Magnetic Properties of the Koidu Kimberlite Complex, Sierra Leone, West Africa     

S. E. Haggerty  R. B. Hargraves  L. A. Tompkins 《Geophysical Journal International》1990,100(2):275-283

  相似文献   

The calculated seismic properties of quartz mylonites with typical fabrics: relationship to kinematics and temperature     

David Mainprice  Martin Casey 《Geophysical Journal International》1990,103(3):599-608

  相似文献   

基桩承载特性的位移协调法分析研究   总被引：1，自引：1，他引：0  

何剑  陈文  曾金艳 《地球科学与环境学报》2003,25(2):27-30

介绍了利用位移协调法分析基桩承载特性的理论基础及计算方法。根据郑州某工程的静载试验资料,求得桩身荷载的传递函数,并利用该函数对基桩承载特性进行了分析。得出了可利用实测传递函数对同一场地的不同桩长、桩径或具有相同工程地质条件的不同场地的基桩进行承载特性分析的结论,以及桩端土层的力学指标和桩身弹模的选取对计算结果有较大影响的结论。  相似文献   

Introducing the near infrared VLTI instrument AMBER to its users     

R.G. Petrov  The AMBER Consortium 《Astrophysics and Space Science》2003,286(1-2):57-67

AMBER is the General User near infrared focal instrument of the Very Large Telescope Interferometer. It is a single mode, dispersed fringes, three telescope instrument. A limiting magnitude of the order of H=13 will allow tackling of a fair sample of extra galactic targets. A very high accuracy, in particular in color differential phase and closure phase modes gives good hope for very high dynamical range observations, possibly including hot extra solar planets. The relatively high maximum spectral resolution, up to 10000, will allow stellar activity observations. Between these extreme goals, AMBER has a wide range of applications including Young Stellar Objects, Evolved Stars, circumstellar material and many others. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Secrets of E2V Technologies CCDs (ex Marconi CCDs)     

Paul R. Jorden  Peter Pool  Simon M. Tulloch 《Experimental Astronomy》2002,14(2):69-75

To complement previously published information on E2V CCDs, we present here some less well-known information about Marconi CCDs. We show details of the performance of deep depletion silicon variants, and discuss other subtleties of performance. We also present an update on L3vision (sub-electron noise) devices, indicating current availability, options, and ongoing development work. Finally, we will give a flavour of the range of custom designs that have been made. Many of these are not commercially available, and may not be familiar to all astronomers or CCD technologists. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

The spectroscopic and interferometric orbit of Gliese 150.2     

Yu. Yu. Balega  A. A. Tokovinin  E. A. Pluzhnik  G. Weigelt 《Astronomy Letters》2002,28(11):773-777

We determined the spectroscopic-interferometric orbit of the binary red dwarf Gliese 150.2 with a period of 13.84 yr and a semimajor axis of 0.257 arcsec. Based on the orbital elements and on accurate measurements of the magnitude difference at several wavelengths, we estimated the spectral types and masses of the components (K0 V and M0 V, 0.79 and 0.55M _⊙) and the dynamical parallax of the binary (40.4 mas).  相似文献   

Paired‐basin comparison of hydrologic response in harvested and undisturbed hardwood forests during snowmelt in central Ontario: II. Streamflow sources and groundwater residence times     

S. S. Monteith  J. M. Buttle  P. W. Hazlett  F. D. Beall  R. G. Semkin  D. S. Jeffries 《水文研究》2006,20(5):1117-1136

  相似文献   

An evaluation of the universal soil loss equation and field techniques for assessing soil erosion on a tropical alfisol in western Nigeria     

P. W. Mtakwa  R. Lal  R. B. Sharma 《水文研究》1987,1(2):199-209

Four techniques for soil erosion assessment were compared over two consecutive seasons for bare-fallow plots and a maize-cowpea sequence in 1985 at IITA, Ibadan, Nigeria. The techniques used were: tracer (aluminium paint), nails (16 and 25), the rill method, and the Universal Soil Loss Equation (USLE). Soil loss estimated by these techniques was compared with that determined using the runoff plot technique. There was significantly more soil loss (P < 0·01) in bare-fallow than in plots under maize (Zea mays) or cowpea (Vigna unguiculata). In the first season, soil loss from plots sown to maize was 40·2 Mg ha^?1 compared with 153·3 Mg ha^?1 from bare-fallow plots. In the second season, bare-fallow plots lost 87·5 Mg ha^?1 against 39·4 Mg ha^?1 lost from plots growing cowpea. The techniques used for assessing erosion had no influence on the magnitude of soil erosion and did not interfere with the processes of erosion. There was no significant difference (P < 0·05) between soil erosion determined by the nails and the runoff plot technique. Soil loss determined on six plots (three under maize, three bare-fallow) by the rill technique, at the end of the season, was significantly lower (P < 0·05) than that determined by the runoff plot technique. The soil loss estimated by the rill method was 143·2, 108·8 and 121·9 Mg ha^?1 for 11, 11, and 8 per cent slopes respectively, in comparison with 201·5, 162·0, and 166·4 Mg ha^?1 measured by the runoff plot method. Soil loss measured on three bare-fallow plots on 10 different dates by the rill technique was also significantly lower (P < 0·01) than that measured by the runoff plot. In the first season the USLE significantly underestimated soil loss. On 11, 11, and 8 per cent slopes, respectively, soil loss determined by the USLE was 77, 92, and 63 per cent of that measured by the runoff plot. However, in the second season there was no significant difference between soil loss determined by the USLE and that determined by the conventional runoff plot technique.  相似文献   

CBERS-1CCD相机飞行绝对辐射标定试验地面同步测量与场地辐射特性分析   总被引：4，自引：1，他引：3  

闵祥军  王志民  傅俏燕  顾英圻 《地球信息科学学报》2002,4(3):43-50

中国对地观测遥感卫星辐射校正场(即敦煌场)位于中国敦煌市西戈壁沙漠的西北角。整个敦煌场地面比较均匀、平坦,面积为30×40km²;测试区(标定区)面积为400×400m²,位于场区的中心位置。2000年8月底至9月初,中国资源卫星应用中心联合安徽光机所在敦煌场地进行了一次CBERS-1CCD传感器飞行绝对辐射标定试验。地表反射率和大气光学特性地面同步测量结果显示:敦煌场地的地面均匀性好,各个通道反射率的变化系数(即相对变化百分比)均小于3%。在可见光、近红外光谱范围内,地面光谱反射率随波长增加逐步增大,例如,在485nm波长处的地面反射率值约为0.18,在830nm波长处的反射率值约为0.26。大气光学特性测量结果显示:0.55μm波长处的大气总光学厚度(≈0.34)和气溶胶光学厚度(≈0.26)相对较小,大气水汽含量也较小。  相似文献