山西临汾盆地黄土剖面重金属分布特征及其影响因素

山西临汾盆地2条黄土剖面重金属分布特征及其影响因素研究表明,Pb、Cu和Zn的垂向变化特征非常相似,而As、Cd和Hg在剖面中的分布特征与前三者不同。各重金属元素在黄土剖面中的变化特征首先均受到黄土源区物质成分的控制,其次不同程度地受到古气候变化的影响。依据Pb、Cu、Zn与各古气候替代性指标(例如磁化率,w(SiO2)/w(Al2O3)等)均呈显著相关,As、Cd和Hg与古气候替代性指标的相关性较差,推断剖面中Cu、Pb、Zn的分布特征受古气候变化的影响,其原因可能主要是这3个金属元素易以类质同象形式赋存在磁性矿物中;而As、Cd和Hg在剖面中的分布特征与古气候无关。但各重金属元素与源区指示元素的相关性表明其在剖面中的分布特征均受黄土源区物质成分的影响和控制。     

应用电性特征研究银川平原地下水水质空间分布规律

以蕴涵丰富地下水系统水循环信息的电性特征为线索,采用电测深法,在分析研究银川平原450 m深度内地下水系统的空间结构的基础上,对平原地下水水质空间分布规律进行了综合研究,为银川平原地下水资源可持续利用战略的制订提供了依据。     

华北地台地热勘探中利用大地电磁测深法(MT)圈定热田范围和探讨地热形成机制

利用大地电磁测深法（MT）反映地质体的电性差异,首先可以确定地质体的空间展布、地质结构和构连;而由于地质体电阻率受地热水影响而降低,进而据此圈定地热水的分布范围;并在此基础上可以进一步探讨地热形成机制。在华北地台地热勘探中MT法取得了较好的勘探效果。     

大别山黄石-六安反射地震剖面新的地质解释

在大别山黄石至六安反射地震剖面上有很多近水平的反射体,表明大别山中心部位的中、下地壳内也有近水平的分层性。反映有流变性和动力学方面的差异,与大型薄皮构造理论对岩石圈性质的认识一致,因而在其运动过程中应服从薄皮构造的运动规律。结合以往对大别山区划分的岩石一构造组合,在前人对此反射地震剖面所作的地质解释的基础上,对反射地震剖面作了较为详细的地质解释,并建立了大别山造山带在此剖面上的两维几何结构。剖面南部为造山过程中形成的背斜构造。地表15km深度内为由碰撞混杂岩组成的扬子与中一朝大陆之间的主滑脱带。剖面中部为造山期后的侵入体。剖面北部为主滑脱带的根带（通常认为的缝合带）,根带被中生代形成的晓天磨子潭断裂带切割。剖面最北端为变质复理石中略晚于主滑脱带的反向冲断带。推溺l下地壳的断开距离在扬子大陆俯冲时（三叠纪前）规模较大,然后逐渐缩小,直至保留到今天的规模。     

The upper mantle structure of the yakutian kimberlite province,eastern Russia

Deep seismic sounding in the region of the Mirnyi kimberlite field indicates that the boundary velocity of the uppermost mantle is elevated (v _b=8.6–8.8 km/sec) and extremely variable near the Mir kimberlite pipe. These velocity heterogeneities are probably associated with the kimberlite magmatism and may be useful in the identification of other kimberlite fields.     

The near infrared camera on the W.M. Keck telescope

The near infrared camera (NIRC) was used for a science demonstration run on the Keck telescope during 16–24 March 1993. The camera used a 256×256 InSb array manufactured by Santa Barbara Research Corporation. Observations were obtained using narrowband and broad band filters from 1 to 2.4 microns, and grisms with a spectral resolution of 0.6 percent in the J, H and K atmospheric windows. The instrument was fully background limited over the entire wavelength range. The sky background was quite low, reaching 14.3 mag/square arc sec in the broadband K _s filter. The image quality of the camera + telescope was excellent, being seeing limited in the range 0.5–0.9.The science demonstration observations of the NIRC on the Keck Telescope included observations of the most distant galaxy known, 4C41.17 at a redshift z=3.8 and the most luminous object known, the IRAS source FSC10214+4724 at a redshift z=2.29. Observations of the radio galaxy address the problem of the alignment effect in high redshift radio galaxies as well as the environments of such systems. FSC10214+4724 appears to be a merging galaxy that is at least 5×10⁸ years old.Based on observations obtained at the W.M.Keck Observatory, which is operated jointly by the California Institute of Technology and the University of CaliforniaThe W.M. Keck Observatory is operated as a scientific partnership between the California Institute of Technology and the University of California. It was made possible by the generous gift of the W.M. Keck foundation and the support of its president, Howard Keck.     

The development of radio astronomy at Hartebeesthoek

The development of radio astronomy at the Hartebeesthoek Radio Astronomy Observatory in South Africa is described. The Hartebeesthoek site was established originally by NASA as one of three Deep Space Stations equipped with 26-m parabolic reflector antennas. It was first used for radio astronomy by South Africa in terms of the NASA host nation agreement which allowed for its use at times when the facility was not needed for its primary purpose of tracking space probes. After NASA withdrew from South Africa in 1975, the South African Council for Scientific and Industrial Research took over the site and the 26-m parabolic reflector antenna, which NASA had abandoned in position, and established it as a national observatory. The development of the facility to the stage where it could support a variety of observing programmes such as continuum observations and mapping, spectroscopy and pulsar timing is described as well as the role played by the Observatory in global programmes of very long baseline interferometry.     

使用价值分析优化方法在功能—技术矩阵求解中的应用

功能—技术矩阵,经众多工作者的努力研究,已渐趋成熟与实用。但如何利用功能—技术矩阵构造在广义现代设计领域中适用的科学模式,解决多学科设计方案的组成与评价问题,还存在薄弱环节。本文利用“使用价值分析优化”的概念,从设计方案技术先进性和经济合理性的协调统一的角度出发,较好地实现了功能—技术矩阵可行优化组合链的组成与评价,弥补了以往的缺陷。     

Airborne gamma-ray spectrometry to quantify chemical erosion processes

Airborne gamma-ray spectrometry data (uranium, potassium and thorium contents) reveal geochemical heterogeneities within the monolithological Hyrôme watershed (ca. 150 km²) in the Armorican massif (western France). Our observations and computations provide important constraints on the spatial distribution and the associated magnitudes of chemical erosion processes at the scale of a small watershed. Two distinct, partially preserved, weathering profiles exhibit a strong correlation between regolith evolution and airborne-derived K/Th ratios, suggesting that the variability is linked to supergene processes. Using both airborne data and laboratory measurements on rock samples, the total net export of potassium has been estimated at 422 ± 50 kg/m² and the chemical weathering rate of potassium at 17 ± 2 kg/km²/a.