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1.
Yu Zhi Shi Xiuzhi Zhou Jian Chen Xin Miao Xiaohu Teng Bing Ipangelwa Timo 《Natural Resources Research》2020,29(2):843-865
Natural Resources Research - A large ore loss and dilution can be expected when using a pre-blast ore boundary for shovel guidance because of the movement and re-distribution of ore in the muck... 相似文献
2.
基于Jason-2高度计2015年地球物理数据集(GDR)38个周期太平洋海域的全球电离层图(GIM)电离层校正值和双频校正值的数据,分不同季度和不同纬度区域比较二者的差异,结果表明:GIM值与双频校正值之间存在明显的差异,GIM校正值普遍高于双频校正值,说明GIM高估了电离层路径延迟,GIM校正值与双频校正值的差异与季节和纬度区间有关。用梯度下降法得到GIM值的修正方程,将修正方程应用于2016年Jason-2的全年数据,修正后的GIM值与双频校正值十分接近,在各年份中均具有良好的适用性。在单频高度计不能使用电离层双频校正算法的情况下,可以利用不同季度和不同纬度区域的修正方程对同等高度的高度计GIM值进行修正以达到双频校正值的精度水平。 相似文献
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郯庐断裂带南段的皖东北地区地质构造复杂,多为厚覆盖区,找矿难度大。由于控矿条件难以调查清楚,缺乏具有区域特色的勘查理论指导,区内金矿勘查长期没有取得突破成果。笔者依托五河金矿整装勘查项目,进行了区域重磁异常特征和成矿规律分析研究,发现皖东北地区北东- 北北东向重力低异常具有弧形条带特征,并以郯庐断裂带为界,大致具有旋转对称性。重磁异常保存印支期构造格架痕迹信息,反映了郯庐断裂带南段时空演化特征,显示了北东- 北北东向主要断裂构造具有继承性,形成于印支期,燕山期继续活动,控制白垩纪“红层盆地”和燕山期成岩成矿作用。中低温热液型金多金属矿床和矽卡岩型铜金矿床是皖东北地区主要矿床类型,均受继承性断裂构造控制。结合郯庐断裂的演化特征,利用物探成果引领地质理论创新,提出了郯庐断裂带南段矿床的“继承性断裂构造控矿模式”。根据继承性断裂构造形成机理分析其空间分布规律,总结了矿化蚀变构造带的物探异常标志,解决了皖东北覆盖区成矿预测与找矿靶区圈定难题,在五河金矿整装勘查区应用取得了重要找矿成果,圈定6个金矿找矿靶区,得到了钻探验证,已发现中型规模金矿床2处、小型3处,估算潜在资源量可达特大型规模,实现了安徽省境内郯庐断裂带金矿找矿的重大突破。 相似文献
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鄂尔多斯盆地马六段在盆地大部分地区被剥蚀,仅在盆地周缘地区分布,因此,有关该盆地马六段白云岩成因研究较少。本文通过对马六段白云岩岩石学特征、阴极发光特征、微量元素特征以及碳氧同位素地球化学特征进行分析,对鄂尔多斯盆地南部马六段白云岩特征及形成机制进行了研究。研究结果表明,盆地南部马六段白云岩主要由细—中晶白云岩组成,白云石具"雾心亮边"结构,阴极发光呈暗红色光。微量元素总体上具有较低的Fe、Mn值,平均值分别为447×10~(-6)和62×10~(-6),较高的K、Na值,平均值分别为517×10-6和252×10~(-6),以及中等含量的Sr元素值,平均值为155×10~(-6)。δ~(13)C值平均为-0.617‰,δ~(18)O值平均为-7.6‰,以上特征均反映出海源流体特征。白云石的"雾心"和"亮边"结构中微量元素含量相差不大,认为是在相同成岩环境的不同成岩阶段形成,其中"雾心"形成于浅埋藏环境的渗透回流白云石化作用,而"亮边"是在深埋藏环境下对早期白云石的调整和加强。 相似文献
6.
Md. Nurul Haider Masahiko Nishimura Minoru Ijichi Ching-chia Yang Wataru Iwasaki Kazuhiro Kogure 《Journal of Oceanography》2018,74(2):197-207
Habitability is defined as an ability of an organism to inhabit different environments. Habitability of organisms, however, cannot be inferred from analyses such as a whole genome or community structures. A recently developed database, the MetaMetaDB, gives us information from what kind of environments one particular 16S rRNA sequence data has ever been obtained, and thus enables us to infer the habitability of the bacterium in question. In order to check the applicability of this database to study the habitability of aquatic bacteria, samples collected at two Naka River stations, one estuarine station from Naka River Estuary, two coastal stations at Oarai in Ibaraki Prefecture, Japan and one station in the Kuroshio Current of the western North Pacific were examined. The phylotypes were tracked against the MetaMetaDB and it was reasonably found that the low-salinity stations were dominated by sequences with “freshwater and groundwater”, “human” and “wastewater” habitat identities, while the high-salinity stations were dominated by those with a “marine” identity. The phylotypes of low-salinity stations with a particular habitat identity were absent or rare in the high-salinity stations and vice versa. The MetaMetaDB also showed that sequences of Cyanobacteria or related phylogenetic groups may be present in the human gut, as well as the probable distribution of the relatives (ancestors/descendants/siblings) of some bacteria. These overall findings proved that the MetaMetaDB is useful as a new tool to infer microbial habitability and it gives us new information on the possible origin and ecology of microorganisms in the environments. 相似文献
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T. Vinutha V. U. M. Rao Bekele Getaneh Molla Mengesha 《Astrophysics and Space Science》2018,363(9):188
In this paper we have studied the anisotropic Kantowski-Sachs, locally rotationally symmetric (LRS) Bianchi type-I and LRS Bianchi type-III geometries filled with dark energy and one dimensional cosmic string in the Saez-Ballester theory of gravitation. To get physically valid solution we take hybrid expansion law of the average scale factor which is a product of power and exponential type of functions that results in time dependent deceleration parameter (\(q\)). The equation of state parameter of dark energy (\(\omega _{\mathit{de}}\)) has been discussed and we have observed that for the three models it crosses the phantom divide line (\(\omega _{\mathit{de}} = -1\)) and shows quintom like behavior. The density of dark energy (\(\rho _{\mathit{de}}\)) is an increasing function of redshift and remains positive throughout the evolution of the universe for the three models. Moreover in Kantowski-Sachs and LRS Bianchi type-I geometries the dark energy density dominates the string tension density (\(\lambda \)) and proper density (\(\rho \)) throughout the evolution of the universe. The physical and geometrical aspects of the statefinder parameters (\(r,s\)), squared speed of sound (\(v_{s}^{2} \)) and \(\omega _{\mathit{de}}\)–\(\omega ^{\prime }_{\mathit{de}}\) plane are also discussed. 相似文献
9.
Using the 2016 Mercury transit of the Sun, we characterize on orbit spatial point spread functions (PSFs) for the Near- (NUV) and Far- (FUV) Ultra-Violet spectrograph channels of NASA’s Interface Region Imaging Spectrograph (IRIS). A semi-blind Richardson–Lucy deconvolution method is used to estimate PSFs for each channel. Corresponding estimates of Modulation Transfer Functions (MTFs) indicate resolution of 2.47 cycles/arcsec in the NUV channel near 2796 Å and 2.55 cycles/arcsec near 2814 Å. In the short (\({\approx}\,1336~\mathring{\mathrm{A}}\)) and long (\({\approx}\,1394~\mathring{\mathrm{A}}\)) wavelength FUV channels, our MTFs show pixel-limited resolution (3.0 cycles/arcsec). The PSF estimates perform well under deconvolution, removing or significantly reducing instrument artifacts in the Mercury transit spectra. The usefulness of the PSFs is demonstrated in a case study of an isolated explosive event. PSF estimates and deconvolution routines are provided through a SolarSoft module. 相似文献
10.
Ayesha Anjum Mousumi Das Jayant Murthy S. B. Gudennavar Rajesh Gopal S. G. Bubbly 《Journal of Astrophysics and Astronomy》2018,39(5):61
We have classified a sample of 37,492 objects from SDSS into QSOs, galaxies and stars using photometric data over five wave bands (u, g, r, i and z) and UV GALEX data over two wave bands (near-UV and far-UV) based on a template fitting method. The advantage of this method of classification is that it does not require any spectroscopic data and hence the objects for which spectroscopic data is not available can also be studied using this technique. In this study, we have found that our method is consistent by spectroscopic methods given that their UV information is available. Our study shows that the UV colours are especially important for separating quasars and stars, as well as spiral and starburst galaxies. Thus it is evident that the UV bands play a crucial role in the classification and characterization of astronomical objects that emit over a wide range of wavelengths, but especially for those that are bright at UV. We have achieved the efficiency of 89% for the QSOs, 63% for the galaxies and 84% for the stars. This classification is also found to be in agreement with the emission line diagnostic diagrams. 相似文献