遥感在新疆淖毛湖戈壁找矿中的应用     

张守林  傅水兴  杨自安 《铀矿地质》2001,17(6):365-367,373

根据不同地质体在不同波段上的光谱特征，选择不同波段的TM数据进行假彩色合成，主成分分析，匹配滤波及多种处理方法，对淖毛湖戈壁琼河坝地区的线环构造特征，赋矿岩层，矿化蚀变等示矿要素进行增强处理和特征提取，取得较好效果，为在戈壁地区快速追踪找矿信息，指导成矿预测提供了重要的基本资料。  相似文献   

羟基磷灰石吸附剂去除铬黄工业废水中铅离子的研究   总被引：14，自引：1，他引：14       下载免费PDF全文

罗惠华  钟康年  刘羽 《岩石矿物学杂志》2001,20(4):587-589

羟基磷灰石吸附剂对铬黄废水中Pb^2 吸附的间歇实验结果表明：当每吨废水中吸附剂用量为200～400g时，常温搅拌60min后，在弱酸性或中性废水中，铅离子质量浓度由2.74mg/L降至0.5mg/L以下，完全符合GB8978-1996工业废水排放标准1.0mg/L。  相似文献   

低地球轨道（LEO）的大型航天器充电     

操学俊  徐跃民 《地球物理学进展》1996,11(3):104-108

本文根据ＬＥＯ中等离子体温度低，密度高，德拜长度小的特点，采用薄鞘层近似，计算了离子收集电流；根据电流平衡方程，考虑表面二次电子发射，计算了大型航天器表面在沉降电子流辐照下的充电特性。  相似文献   

上行离子密度分布特性的理论研究          下载免费PDF全文

史建魁  刘振兴 《地球物理学报》1996,39(2):159-168

采用动力学方程，求解了定态情况下磁层中上行离子沿磁力线的分布函数，针对不同的Ｋ_ｐ指数，分别对北半球极光带区起源的上行离子Ｏ_＋、Ｈ_＋和Ｈｅ_＋在子午面内沿磁力线的密度分布及其特性进行了研究．结果表明：１．沿磁力线向外，上行离子密度在近地空间呈急剧下降趋势，在远地空间呈缓慢下降趋势；２．重离子或初始能量较小的离子，其密度沿磁力线向外下降较快；３．Ｋ_ｐ指数越大，离子进入磁层的空间范围越大；４．离子的投掷角分布对密度分布的影响甚小；５．离子密度沿磁力线的下降程度随到Ｘ轴距离的增大而呈增大趋势；６．在典型参数条件下，求得上行离子Ｏ_＋在等离子体片边界附近的密度为１０^－３－１０^－２个ｃｍ^－３，这与观测结果相一致．  相似文献   

彩色合成选择法及其在黄河入海口研究中的应用     

张昭贵 《遥感学报》1992,(4)

彩色合成选择法是根据色度学原理,求出地物之间在各种彩色合成方案中的色差,以选择彩色合成方案。将此方法应用到黄河入海口,提取黄河水、海水、沙滩、陆地等主要地物信息,效果明显。  相似文献   

载金石英的化学成分特征及其意义     

胡大千  贺义兴 《吉林大学学报(地球科学版)》1992,(1)

利用电子显微镜(EM)及能谱仪(EDS),分析研究了变生热液形成的载金石英的化学成分、离子扩散作用以及金在石英中的赋存状态等问题,探讨了它们的形成和变化机理。研究结果表明:Al~(3+)、Ti~(3+)、TFe、Na~(+)、K~(+)、Ca~(2+)等在石英中为类质同像混入物;石英和黄铁矿之间的离子相互扩散作用,表现为石英中Al离子的带出和Fe离子的带入,黄铁矿中Fe离子的带出和Al离子的带入;石英中呈分散状态分布的金主要为离子金,它们充填在石英结构中,起平衡电价的作用。  相似文献   

Surface complexation at hydrous fluorapatite     

Willis Forsling  Liuming Wu 《Aquatic Sciences - Research Across Boundaries》1993,55(4):336-346

The adsorption of H⁺, OH^– and ARS (Alizarin Red S) onto hydrous fluorapatite surfaces and Ca²⁺—ARS complexation in solution were studied by means of combined potentiometric and spectrophotometric titrations, as well as zeta potential and FT-IR measurements. Corresponding equilibrium constants of surface and solution reactions are determined. The application in flotation processes is discussed.  相似文献   

Distribution of ionospheric O<Superscript>+</Superscript> ion in synchronous altitude region     

Jiankui?Shi?Email author  Zhenxing?Liu  Zhang?T.?L.  Jianshan?Guo  Manlian?Zhang  Sheping?Shang  Xigui?Luo 《中国科学D辑(英文版)》2003,46(10):986-993

Based on satellite observation data, using dynamics equation, the ionospheric O⁺ ion’s distribution in the synchronous altitude region for different geomagnetic activity indexK _p is studied by theoretical modeling and numerical analyzing, and semi-empirical models for the O⁺ ion’s density and flux versus longitude in the synchronous altitude region for differentK _p are given. The main results show that in the synchronous altitude region: (i) The O⁺ ion’s density and flux in day-side are larger than those in nightside. (ii) With longitude changing, the higher the geomagnetic activity indexK _p is, the higher the O⁺ ion’s density and flux, and their variation amplitude will be. The O⁺ ion’s density and flux whenK _{p ≥} 6 will be about ten times as great as that whenK _p = 0. (iii) WhenK _p = 0 orK _{p ≥} 6, the O⁺ ion’s density reaches maximum at longitudes 120° and 240° respectively, and minimum in the magnetotail. WhenK _p = 3−5, the O⁺ ion’s density gets to maximum at longitude 0°, and minimum in the magnetotail. However, the O⁺ ion’s flux reaches maximum at longitude 120° and 240° respectively, and minimum in the magnetotail for anyK _p value.  相似文献   

Sodium emission from Comet Shoemaker-Levy 9 in the magnetosphere of Jupiter     

V. V. Prokof’eva  V. P. Tarashchuk  Yu. T. Tsap 《Astronomy Letters》2002,28(2):130-138

On July 20, 1994, before the Q fragments of Comet Shoemaker-Levy 9 fell to Jupiter, more than 200 spectra of the Jovian features were obtained at the Crimean Astrophysical Observatory in the wavelength range 5700–7600 Å with a 26 s exposure time and a spectral resolution of 20 Å. We found a time-varying Na D line emission in the form of two components with Doppler shifts of about 30 Å. The brightest and most frequent sodium flares were detected when the Q fragments passed through the Jovian inner magnetosphere at a distance of about three the Jovian radii (3R_J) from its center, where they crossed the Io-Jupiter current tube. A frequency analysis of our data revealed a flare recurrence time scale of 1 min. We conclude that sodium was released from the cometary dust and from the surfaces of numerous cometary debris and that its amount was enough to produce the observed emission. The observed high-speed clouds of sodium atoms are assumed to have been formed through ionization, ion acceleration by the bidirectional electric fields of Alfvén waves in the Io-Jupiter current tube, and their neutralization.  相似文献   

Evolution of Ore-Forming Fluids and Ag-Cu Polymetal Mineralization in the Lanping Basin, Yunnan   总被引：1，自引：0，他引：1  

Wang C. S.  Tang J. X.  Gu X. X.WT  ”BX 《地学前缘》2000,(Z1)

EVOLUTION OF ORE-FORMING FLUIDS AND Ag-Cu POLYMETAL MINERALIZATION IN THE LANPING BASIN, YUNNAN“KeyProjectforResourcesandEconomics” (95 0 2 0 0 1 0 1)oftheMinistryofLandResources  相似文献