草莓红绿柱石(Pezzottaite)的晶体结构测定及其意义

利用CCD单晶衍射仪对草莓红绿柱石进行晶体结构测定,测定其空间群为R3c,并讨论了结构中Li 有序地置换Be2 造成c/a值的变化特征。晶体中发现复三方偏三角面体的负晶包裹体,其宏观对称属m,它与空间群Rc相对应,但与测出晶体结构的空间群有矛盾。X射线结构测定已否定了其空间群为Rm的看法。要解决草莓红绿柱石晶体空间群是否有对称中心(Rc或Rc)的问题,还需进一步将X射线结构的数据及其有关的电性实验结合分析。     

盘江火铺煤矿矸石场滑坡预警、征兆特征及其防治

本文通过火铺煤矿矸石场滑坡的调查研究,在对其地质环境条件分析的基础上,论述滑坡的特征,探讨其形成机制,提出了防治措施,可供该矿山地质环境的保护与修复参考。     

贵州绥阳双河洞国家地质公园洞穴基本特征及成因探讨

106地质大队于1959～1960年曾对双河洞石膏矿进行过地质勘查。1986年～2006年4月,先后有中、法、日等国专家19次进双河洞考察,初步查明了该洞总长度为105.7km,是亚洲第二长洞,在世界上排名第16位。该洞不仅规模宏大,网络复杂,且有一定数量的次生淋滤型石膏矿分布,成为国内外罕见的独特洞穴景观。双河洞自2004年荣获国家地质公园称号以来,已引起国内外专家的广泛关注。该洞的形成,与该区域大范围内下寒武统清虚洞组上部至中寒武统平井组下部白云岩中,含大量硬石膏层有着密切的成因联系。     

滇西南澜沧江结合带北段云县花岗岩的地质特征及形成环境

滇西南澜沧江结合带云县花岗岩体的岩石类型主要为黑云二长花岗岩,SiO2含量平均为68.57%,K2O/Na2O值平均为1.67,相对富钾,岩石属高钾钙碱性系列,岩石酸、碱度低于同类岩石平均值,而镁铁组分高于平均 值,显示岩石偏中性,与同碰撞构造环境形成的花岗岩特征类似.Al2O3含量较高,平均为13.66%,A/CNK平均为1.1,呈铝过饱和,CIPw计算结果均出现标准矿物刚玉分子(105).岩石总体上相对富集大离子亲石元素,亏损高场强元素.稀土元素总量较高,平均为240.75×10-6,轻稀土元素富集,重稀土元素亏损,(La/Yb)N为8.88～9.41,分异不是很大,Eu为中等负异常,銭u为0.52～0.57.经多种相关图解判别,岩石属S型花岗岩,其构造环境相当于大陆碰撞花岗岩类(CCG).锆石颗粒U-Pb测年结果显示,源岩的形成年龄最晚是晋宁期(778 Ma),岩体主体形成于华力西晚期一印支期.其中岩浆成因锆石样品的206Pb.238U和207Pb/235U年龄分别为49 Ma和61 Ma,反映在云县岩体中可能存在喜马拉雅期岩浆活动.     

Cyclotron amplification of geomagnetic micropulsations Pc1 in the magnetosphere

A numerical analysis of cyclotron instabilities is carried out by computing the dispersion relation for a three component cold plasma-beam system. Rates of growth and damping for various values of the stream density are calculated from the dispersion relation. The rates of growth and damping increase monotonically as the number density of the proton stream increases. It is found that the frequencies at the rates of maximum growth and the damping decrease slightly to lower frequencies and a sharp peak at these frequencies becomes blunt. The minimum e-folding times of an ion cyclotron wave for (a) σ_s = 10⁻⁴, σ_i = 10⁻² and (b) σ_s = 10⁻¹, σ_i = 10⁻² are about 3·84 and 0·16 sec respectively in the vicinity of the equatorial plane at 6 Re, where σ_s and σ_i are the ratios of the beam density N_s and the helium ion (H₆⁺) density N_i to the total positive ions in the plasma-beam system.     

Variations in exospheric density at heights near 1100km, derived from satellite orbits

In an earlier paper, values of exospheric density were obtained from the orbit of Echo 2 for the years 1964–1965. The results indicated a semi-annual variation in density by a factor of between 2 and 3, considerably larger than predicted by existing atmospheric models.

These studies have now been extended to the beginning of 1967, using both Echo 2 and Calsphere 1, to show how the density is responding to increasing solar activity. Variations in density during 1964 have been analysed in more detail. The long-term variation associated with the solar cycle and the short-term variations associated with magnetic and solar disturbances agree with the variations expected on the basis of current models. The semi-annual variation is persisting to higher levels of solar activity, and although its amplitude is diminishing the factor of variation was still 1.6 in 1966.     

Measurements of radio noise at 0.700 mc and 2.200 mc from a high-altitude rocket probe

Radio noise observations at frequencies of 0·700 Mc and 2·200 Mc were made at altitudes between 3000 and 11,000 km from a Blue Scout Jr. high-altitude rocket probe on 30 July 1963. A steady background flux of (7·5₋₃⁺⁶) × 10⁻¹⁹ W m⁻²)(c/s)⁻¹ at 0·700 Mc and (1·8^+1.0_−0.5 × 10⁻¹⁹ W m⁻² (c/s)⁻¹ at 2·200 Mc was observed. Assuming a galactic origin of the observed fluxes at both frequencies, the averaged sky brightnesses are b(0·700 Mc) = (6₋₃⁺⁵) × 10⁻²⁰ W m⁻² (c/s)⁻¹ sr⁻¹b(2·200 Mc) = (1.4^+1.0_−0.5 × 10⁻²⁰ W m⁻² (c/s)⁻¹ sr⁻¹ The observed brightness at 2·200 Mc is in reasonable agreement with the results of other observers. The apparent brightness at 0·700 Mc is, however, greater than was expected from previous observations. An alternative source of the 0·700 Mc flux in the terrestrial exosphere, as well as characteristics of several noise bursts observed during the flight, is briefly discussed.