《西北地质》2001～2012年总被引频次的统计与分析

期刊的总被引频次在期刊的统计与分析中是十分重要的,笔者利用中国科学技术信息研究所出版的《中国科技期刊引证报告》(核心板)(CJCR)和万方数据出版的《中国期刊引证研究报告》(扩展版)(WD)等二家比较著名的统计机构的统计数据,对《西北地质》总被引频次进行了统计与分析。为了不断提高《西北地质》的办刊质量,笔者重点对《西北地质》2001~2012年的总被引频次及相关数据进行了统计与分析。结果表明:《西北地质》从2001~2012年在《中国科技期刊引证报告》(核心版)中的总被引频次增加了416,总被引频次增长率为660.32﹪。《西北地质》从2003~2012年在《中国科技期刊引证报告》中的总被引频次增加了782,总被引频次增长率为1133.33﹪。事实说明,《西北地质》多年来总被引频次一直在稳步上升。最后,笔者分析了影响期刊总被引频次的因素,对如何提高期刊的总被引频次提出了合理化的建议。     

Comprehensive Development and Utilization of Saline Lake Groups in Dingbian,Shanxi Province of China

正The Dingbian Saline Lake groups are in Dingbian County,northwest of Shaanxi province,and located on the border area of the Loess Plateau and Maowusu Desert in Northern Shanxi.It's altitude is more than 1300m.The     

Recent Progresses in Comparative Planetology——Summary of the Session of Comparative Planetology at the 3rd Conference of Earth System Sciences

Comparative planetology is an interdisciplinary science between Earth sciences and astronomy. It studies physical, chemical and dynamical properties of planets and satellites and their surface characteristics, interior structures and chemistry, magnetic field, climate and possible existence of life. Although the study of comparative planetary science is at its infancy stage in China, it is very encouraging to see that 25 papers were received by the session, which is much more than what we expected. It indicates that more and more scientists are interested in this research field. These papers can be classified into three categories: solar planets, extra-solar planets, and moon explorations. Scientists from both China and oversea reported their recent results.     

中国资源外交的地缘政治分析

资源外交寓于国际地缘政治的长期博弈之中。地缘政治是一国对外交往所要考虑的重要因素之一。本文立足于内线周边和外线外围的地缘关系分析,总结了中国资源外交地缘政治的总体态势和潜在风险,并试图提出我国资源外交的基本思路。在全球地缘政治格局中,中国的资源外交包括内线地带和外线地带两个层次：内线由接壤的邻国以及接近的近邻组成,是中国资源外交的战略依托地带;外线由涵盖美洲、欧洲、非洲和澳洲大陆的资源生产大国和消费大国组成,是中国资源外交的战略腾挪空间。在这两个层次上,我国的地缘风险主要来自其他大国的地缘战略遏制、“走出去”战略的地缘选择权旁落、资源通道和贸易路线受制于人。要突破这些地缘限制与束缚,我国的资源外交需统筹国内、国际两个大局,分清内线、外线战略方向的轻重缓急,以周边关系为首要、以大国关系为关键、以发展中国家关系为基础,积极拓展对外友好关系的发展空间,有序扩展资源合作领域,坚定维护国家资源权益。     

The disappearance of eclipses in the central star of the planetary nebula NGC 2346

This paper gives the result of photographic photography of the central star AGK3-0° 695 of the planetary nebula NGC 2346 made from 1981 through 1987. From it we see that after the large-amplitude eclipses which had started at the end of 1981 had continued for several years, the amplitude began to decrease rapidly in 1986 to ˜1.1 mag from ˜4 mag in 1984. In 1987, only irregular fluctuations with amplitudes ˜0.4 mag were present in the light curve and not longer any clear periodicity. A preliminary analysis of this phenomenon is carried out here.     

Ground-based near infrared spectroscopy of Jupiter's ring and moons

The backscattered reflectivity of Jupiter's ring has been previously measured over distinct visible and near infrared wavelength bands by a number of ground-based and spaceborne instruments. We present spectra of Jupiter's main ring from 2.21-2.46 μm taken with the NIRSPEC spectrometer at the W.M. Keck observatory. At these wavelengths, scattered light from Jupiter is minimal due to the strong absorption of methane in the planet's atmosphere. We find an overall flat spectral slope over this wavelength interval, except for a possible red slope shortward of 2.25 μm. We extended the spectral coverage of the ring to shorter wavelengths by adding a narrow-band image at 1.64 μm, and show results from 2.27-μm images over phase angles of 1.2°-11.0°. Our images at 1.64 and 2.27 μm reveal that the halo contribution is stronger at the shorter wavelength, possibly due to the redder spectrum of the ring parent bodies as compared with the halo dust component. We find no variation in main ring reflectivity over the 1.2°-11.0° phase angle range at 2.27 μm. We use adaptive optics imaging at the longer wavelength L′ band (3.4-4.1 μm) to determine a 2-σ upper limit of 22 m of vertically-integrated I/F. Our observing campaign also produced an L′ image of Callisto, showing a darker leading hemisphere, and a spectrum of Amalthea over the 2.2-2.5 and 2.85-3.03 μm ranges, showing deep 3-μm absorption.     

Fluid dynamics of local martian magma oceans

The evolution of a melt region produced by a large impact during Mars formation is addressed. While some impact induced melt is redistributed during crater excavation, sufficiently large impacts (much larger than basin forming impacts) generate an intact melt region which is retained beneath the excavation zone, i.e., a local magma ocean. Local magma ocean evolution depends on the effective rheology controlling large scale deformation of the solid part of the planet, mechanism of crystallization, and melt region size. Within the uncertainties of various parameters, two scenarios are possible. For sufficiently weak rheology or large melt region size, evolution is characterized by rapid extrusion and formation of a global magma ocean. For sufficiently strong rheology or small melt region size, in situ crystallization to a partially molten solid state occurs prior to isostatic adjustment. Subsequent to in situ crystallization, local magma ocean evolution depends on melt region size and efficiency of lateral redistribution compared to bulk conductive cooling. For large melt regions, lateral spreading occurs via plastic deformation and results in an asymmetric, global, partial melt layer. For small melt region size, viscous spreading viscous can result in bulk cooling below the solidus prior to formation of a global layer. A hypothesis for the origin of the hemispherical crustal dichotomy and Tharsis rise is suggested. The dichotomy is associated with a global partial melt layer produced by evolution of a large, local magma ocean. After dichotomy formation, evolution of a second, smaller, local magma ocean is related to Tharsis development.     

蒙特卡罗法在资源评价中的应用

结合陕西灞源地区金矿预测实例,探讨了在蒙特卡罗法应用中潜在矿床总数估计及资源总量概率分布向资源潜力分布转换两个环节的合理实现方法。在一定条件下,矿点空间分布模型和发现过程模型可有效地用于估计潜在矿床总数。通过坐标平移或求截尾分布而将资源总量的概率分布转变为资源潜力的概率分布,可得到较为符合地质实际的评价结果。