Modeling Virgin Compression of Reconstituted Clay at Different Initial Water Contents     

卞夏  钱森  丁建文 《海洋工程》2015,29(5):745-755

The observations on compressibility of reconstituted clays show that the compression line with a higher initial water content lies above the compression line with a lower initial water content for a given clay. Hence there exists additional void ratio due to initial water contents among virgin compression lines (VCLs) of reconstituted clays. In this paper, the difference in void ratio caused by different initial water contents is investigated based on the empirical equation proposed by Liu and Carter (2000) for describing the differential void ratio at the same stress between natural and reconstituted clays. The mechanism of compressibility of reconstituted clays, when the stress level is larger than the remolded yield stress, is also discussed.  相似文献   

Environmental dependence of stellar mass and stellar velocity dispersion of CMASS galaxies     

X.‐F. Deng 《Astronomische Nachrichten》2015,336(10):1017-1024

In this study, I attempt to apply for a new statistical method and investigate the environmental dependence of stellar mass and stellar velocity dispersion in the CMASS sample of the Sloan Digital Sky Survey Data Release 9 (SDSS DR9). I divide the CMASS sample with redshifts 0.44 ≤ z ≤ 0.59 into many subsamples with a redshift binning size of Δz = 0.01, and analyze the environmental dependence of stellar mass and stellar velocity dispersion of subsamples in each redshift bin. It is found that stellar mass and stellar velocity dispersions of CMASS galaxies are very weakly correlated with the local environment. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Leaf chlorophyll constraint on model simulated gross primary productivity in agricultural systems     

《International Journal of Applied Earth Observation and Geoinformation》2015

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基于作物缺水指数的土壤含水量估算方法   总被引：1，自引：0，他引：1  

虞文丹  张友静  郑淑倩 《国土资源遥感》2015,(3)

为研究江苏省徐州市的土壤水分时空分布及动态变化,基于MODIS数据和站点气象数据,利用蒸散发双层模型和考虑土壤水分可供率的改进双层模型分别计算实际蒸散发量,利用Penman-Monteith模型计算区域潜在蒸散发量,计算获得作物缺水指数(crop water stress index,CWSI),并与2010年7月和11月的土壤相对含水量实测数据分别进行回归分析建模,得到了土壤含水量分布图。结果表明:基于蒸散发双层模型的土壤含水量估算结果与实测值的决定系数分别为0.53和0.72,平均相对误差分别为5.89%和9.6%;对双层模型进行改进后,土壤含水量估算结果与实测值的决定系数都为0.84,平均相对误差分别为3.47%和6.03%,利用改进后的双层模型对土壤相对含水量进行估算效果更好。  相似文献   

云微物理参数的地基探测反演研究综述   总被引：1，自引：1，他引：0  

程周杰  王洪芳  白洁 《气象科技》2007,35(1):9-14

云相态、云滴谱分布和云液态水含量作为重要的云微物理参数,对气候变化、天气变化、人工影响天气和飞行安全等很多方面都有着重要的影响。云微物理参数的研究已是国际气象学研究领域中的热点之一,而在国内这方面的研究较少。简要论述了地基方法在云微物理学研究的优越性,扼要总结了国内外地基探测技术的发展现状,重点概括了云相态、云滴谱和云液态水3个参数的地基反演算法,并予以评价,展望了未来发展趋势,为国内云微物理研究提供了参考与借鉴。  相似文献   

Stellar populations in barred spirals     

Simon Cantin  Carmelle Robert  Anne Pellerin  Mercedes Moll 《New Astronomy Reviews》2006,49(10-12):536

OASIS observations obtained at the Canada–France–Hawaii Telescope for the spiral galaxies NGC 4900 and NGC 5430 produce one spectrum for each 0.41″ element of the 11″ × 15″ field of view. This allows for the spatial characterisation of the different stellar populations. From these observations we study the young (10 Myr) and older stellar populations using evolutionary synthesis codes. Based on the gas emission lines, we find that the young populations are located in relatively small regions and dominate the integrated flux. In NGC 4900, the young populations are distributed in a bar-like structure featuring a hole near the position of the galaxy’s centre. The young stellar populations of NGC 5430 form a nuclear ring and two patches at the base of the spiral arms. Based on Mg₂ and FeI absorption lines, we find that in both galaxies, the young stars are superimposed on a relatively homogenous population of a few Gyr.  相似文献   

基于电离层电子含量变化率的周跳探测方法     

崔建勇  陈明剑  雷娜娜 《全球定位系统》2012,37(3):37-40,52

推导了利用GNSS双频数据的基于电离层电子含量(TEC)变化率的周跳探测方法,分析了电离层平静期和活跃期的TEC变化率,并认为对1s采样率的数据来说无论是否发生电磁暴都不影响TEC变化率法的使用,通过实验证明TEC变化率法能对1s采样率数据中的、其它周跳探测方法较难探测的小周跳进行探测,而联合利用TEC变化率法和MW法可对各自不敏感的周跳组合进行有效探测,实验证明:联合法对电离层平静期和活跃期中、采样间隔为1s的数据中的周跳都具有很高的探测成功率。  相似文献   

盐酸浓度和用量对粘土沉积物硼的提取和同位素组成的影响   总被引：2，自引：2，他引：0       下载免费PDF全文

张艳灵  肖应凯  马海州  马云麒  罗重光 《盐湖研究》2012,20(3):21-25,31

研究了处理粘土沉积物时不同浓度盐酸和用量对溶出硼量及硼同位素组成的影响。结果表明,粘土沉积物中硼的溶出量随盐酸浓度的增加而增加,当盐酸浓度相同时,溶出的硼量随所加盐酸用量的增加而增加,加热有利于硼的溶出。实验结果还表明,粘土沉积物硼的溶出量对测定的硼同位素组成没有明显的影响。  相似文献   

Star formation in the LMC: Comparative CCD observations of young stellar populations in two giant molecular clouds     

J. Ruppert  H. Zinnecker 《Astronomische Nachrichten》2009,330(8):773-783

This work deals with a CCD imaging study at optical and near‐infrared wavelength oftwo giant molecular clouds (plus a control field) in the southern region of the Large Magellanic Cloud, one ofwhich shows multiple signs of star formation, whereas the other does not. The observational data from VLT FORS2 (R band) and NTT SOFI (Ks band) have been analyzed to derive luminosity functions and color‐magnitude diagrams. The young stellar content of these two giant molecular clouds is compared and confirmed to be different, in the sense that the apparently “starless” cloud has so far formed only low‐luminosity, low‐mass stars (fainter than m_Ks ∽ 16.5 mag, not seen by 2MASS), while the other cloud has formed both faint low‐mass and luminous high‐mass stars. The surface density excess oflow‐luminosity stars (∽2 per square arcmin) in the “starless” cloud with respect to the control field is about 20% whereas the excess is about a factor of 3 in the known star‐forming cloud. The difference may be explained theoretically by the gravo‐turbulent evolution of giant molecular clouds, one being younger and less centrally concentrated than the other (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Stellar mass estimates in early-type galaxies: procedures, uncertainties and models dependence     

M. Longhetti  P. Saracco 《Monthly notices of the Royal Astronomical Society》2009,394(2):774-794

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