岩石圈深部的水及其意义探讨   总被引：1，自引：0，他引：1  

王方正  胡宝群 《地质科技情报》2000,19(4):25-30

在对水的相图、典型地区的地温曲线、矿物的脱水行为及一些矿物和岩石的含水量等研究的基础上指出,以１５．５～２５．１ｋｍ深度为界,在该深度以上的岩石圈浅部水是液态,而在该深度以下的岩石圈深部水是气态,水以矿物的结构水形式被带入到１５．５～２５．１ｋｍ深度以下的岩石圈中,若矿物结构水完全脱出,在储冲带中水临界温度至矿物脱结构水的极限温度相对应的的区域内（如秦岭１５．５～６４．０ｋｍ）,平均含水量的０．５～１．０％,讨论了在岩石圈深部矿物脱水作用与局高压环境、高导低速带之间的成因联系。  相似文献   

氯化钾与硫酸钠制硫酸钾工艺的优化          下载免费PDF全文

屠兰英  赵启文 《盐湖研究》2000,8(3):32-39

根据 K+ ,Na+∥ Cl-,SO4 2 -— H2 O体系相图 ,提出了氯化钾与芒硝制备硫酸钾工艺中新的工业化生产循环和解决钾芒硝富集问题的具体方案 ,取得良好效果。  相似文献   

非规则网带断层地震数据的网格化   总被引：4，自引：0，他引：4  

张美根  乌达巴拉 《地球物理学进展》1999,14(1):69-77

非规则网地震勘探中,由解释人员解释出来的层位信息包括大量不规则分布的高程数据和断层构造的断点数据,因而其构造图成图的网格化是一件相当复杂而又难度较大的工作,本文较全面地研究了非规则网带断层地震数据的网格化过程（本文针对是正断层情况）,提出了一种快速实用的正方形网格化方法,经对实际资料处理证明,它能够适用于非常复杂的情况,并且处理效果理想。  相似文献   

UBVI CCD photometry of M35 (NGC 2168)     

H. Sung †  M. S. Bessell † 《Monthly notices of the Royal Astronomical Society》1999,306(2):361-370

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The ages of pre-main-sequence stars     

Christopher A. Tout  Mario Livio  Ian A. Bonnell 《Monthly notices of the Royal Astronomical Society》1999,310(2):360-376

The position of pre-main-sequence or protostars in the Hertzsprung–Russell diagram is often used to determine their mass and age by comparison with pre-main-sequence evolution tracks. On the assumption that the stellar models are accurate, we demonstrate that, if the metallicity is known, the mass obtained is a good estimate. However, the age determination can be very misleading, because it is significantly (generally different by a factor of 2 to 5) dependent on the accretion rate and, for ages less than about 10⁶ yr, the initial state of the star. We present a number of accreting protostellar tracks that can be used to determine age if the initial conditions can be determined and the underlying accretion rate has been constant in the past. Because of the balance established between the Kelvin–Helmholtz, contraction time-scale and the accretion time-scale, a pre-main-sequence star remembers its accretion history. Knowledge of the current accretion rate, together with an HR-diagram position, gives information about the rate of accretion in the past, but does not necessarily improve any age estimate. We do not claim that ages obtained by comparison with these particular accreting tracks are likely to be any more reliable than those from comparisons with non-accreting tracks. Instead, we stress the unreliability of any such comparisons, and use the disparities between various tracks to estimate the likely errors in age and mass estimates. We also show how a set of coeval accreting objects do not appear coeval when compared with non-accreting tracks. Instead, accreting pre-main-sequence stars of around a solar mass are likely to appear older than those of either smaller or larger mass.  相似文献   

论CILa/CISm—CILa图解     

万渝生 《现代地质》1990,4(3):81

通过对分离结晶作用和批式熔融作用C_l^y/C_l^x-C_l^y图解的数学分析,笔者认为,虽然C_l^La/C_l^sm-C_l^La图解在一定程度上能区分这两种不同岩浆作用过程,但是,Treuil等的解释是不完全的。直线的斜率和截距还极大地受参数C_o^x,C_o^y,D_x,D_y的影响。该图解并非总是有效。本文还给出了一般式C_l^y/C_l^x-C_l^y在其它方面的可能应用。  相似文献   

地理知识可视化中知识图特征与应用——以小流域淤地坝系规划为例   总被引：1，自引：0，他引：1  

龚建华  李亚斌  王道军  黄明祥  王伟星 《遥感学报》2008,12(2):355-361

依据心智表达的双重编码理论、地理的空间图形思维特点以及支持可视化知识探析需求,讨论地理知识可视化中知识图的定义与特点,并把地理知识图分为地理概念命题图与地理相似图解图,地理相似图解图又可分为逻辑拓扑相似图、空间结构相似图、变量关系相似图以及地理过程相似图.以黄土高原的小流域淤地坝系规划为案例,研究了支持坝系空间规划知识图中的概念命题图与相似图解图的形式、种类及其相互关系.  相似文献   

1992-2014年河北省流动重力资料整理     

张娜  龚燕民  苏树朋  李博 《地震地磁观测与研究》2017,38(2):112-119

系统整理河北省1992-2014年流动重力资料,利用LGADJ数据处理软件,对每期重力数据进行单期平差、多期整体平差计算,改正历史遗留问题,利用差分结果绘制145幅流动重力等值线差分图,通过具体异常点位及重力变化分析,得出：①地震前重力场变化强度与震级大小存在相关性;②流动重力观测资料地震前具有较为明显的前兆异常反应;③地震均发生在重力变化的“0”等值线附近地区。  相似文献   

上海市主体功能区划分与综合制图     

花叶  刘海燕 《地理空间信息》2010,8(6):123-125

以《上海市主体功能区划图集》的数据处理、内容结构设计、地图设计与制作工艺等不同阶段遇到的问题及解决方案为例,探讨了此类反映总体规划、区域划分类地图(集)的设计特点与关键技术。  相似文献   

Threshold of motion of bivalve and gastropod shells under oscillatory flow in flume experiments     

Cristiano Fick  Eduardo Puhl  Elírio Ernestino Toldo Jr 《Sedimentology》2020,67(1):627-648

The threshold of motion of non-fragmented mollusc shells was studied for the first time under oscillatory flow. In this regard, flume experiments were used to investigate the threshold of motion of three bivalve and three gastropod species, two typical mollusc classes of coastal coquina deposits. The sieve diameters ranged from 2·0 to 15·9 mm. These experiments were performed on a flat-bottom setup under regular non-breaking waves (swell) produced by a flap-type wave generator. The critical Shields values for each species of mollusc were plotted against the sieve and nominal diameter. Moreover, the dimensionless Corey shape factor of the shells was evaluated in order to investigate the effect of mollusc shell shapes on the threshold of motion. According to their critical Shields parameter, the mollusc threshold data under oscillatory flow present smaller values than the siliciclastic sediments when considering their sieve diameter. In addition, the mollusc datasets are below the empirical curves built from siliciclastic grain data under current and waves. When considering the nominal diameter, the critical Shields parameter increases and the mollusc data are closer to siliciclastic sediments. Bivalves, which have a flat-concave shape (form factor: 0·27 to 0·37), have a higher critical Shields parameter for smaller particles and more uniform datasets than the gastropod scattered data, which have a rounded shape (form factor: 0·58 to 0·62) and have varied morphologies (ellipsoidal, conical and cubic). The comparison between previous current-driven threshold data of bioclastic sediment motion and the data of mollusc whole shells under oscillatory flow shows a fair correlation on the Shields diagram, in which all datasets are below the mean empirical curves for siliciclastic sediments. These findings indicate that the shape effect on the transport initiation is predominant for smaller shells. The use of the nominal diameter is satisfactory to improve the bioclastic and siliciclastic data correlation.  相似文献