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91.
Much of the authors' knowledge of kin interaction and exchange in Britain is partial, in that it is based on studies of co-resident groups and excludes consideration of kin "beyond the household". It is known that there have been large declines in intergenerational co-residence, raising fears that family bonds have weakened. It is also commonly assumed that family members are less likely to live in close proximity than in the past. In this paper the authors examine one important aspect of kin relationships--proximity of adult children to their parents--using nationally representative data from 1986, 1995, and 1999. The analyses presented focus on: differences between 1986, 1995, and 1999 in proximity of adults to their parents; sociodemographic characteristics associated with variations in proximity, and temporal differences in the pattern of these variations. The paper concludes with an assessment of some of the policy implications of the findings.  相似文献   
92.
This paper discusses the dispersal of facilities where family members migrate to different destination countries. Terminology for internationally dispersed families is proposed, and the term branch migration is suggested for the migration of related people from the same source country to different destination countries. Data from two 1993 surveys of senior secondary students show that 22% of Sydney students and 20% of Hong Kong students have relatives in two or more other countries. The data suggest that many Asian migrant families have branched between the US, Canada, Australia and other migrant-receiving nations. The causes and implications of the international dispersal of families are discussed.  相似文献   
93.
I present the first results from a Hubble Space Telescope/NICMOS imaging study of the most metal-poor blue compact dwarf galaxy, I Zw 18. The near-infrared color-magnitude diagram (CMD) is dominated by two populations, one 10-20 Myr population of red supergiants and one 0.1-5 Gyr population of asymptotic giant branch stars. Stars older than 1 Gyr are required to explain the observed CMD at the adopted distance of 12.6 Mpc, showing that I Zw 18 is not a young galaxy. The results hold also if the distance to I Zw 18 is significantly larger. This rules out the possibility that I Zw 18 is a truly young galaxy formed recently in the local universe.  相似文献   
94.
We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain the geometry of the universe. Within the class of cold dark matter models, we find that the overall fractional energy density of the universe Omega is constrained to be 0.85相似文献   
95.
We have examined the fluid inclusion data and fluid chemistry of Australian orogenic and intrusion-related gold deposits to determine if similar mineralization processes apply to both styles of deposits.The fluid inclusion data from the Yilgarn craton,the western subprovince of the Lachlan orogen,the Tanami,Tennant Creek and Pine Creek regions,and the Telfer gold mine show that mineralization involved fluids with broadly similar major chemical components(i.e.H_2O NaCl CO_2±CH_4±N_2).These deposits formed over a wide range of temperature-pressure conditions(<200 to>500℃,<100~400MPa).Low salinity, CO_2-bearing inclusions and low salinity aqueous inclusions occur in both systems but the main difference between these two types of deposits is that most intrusion-related gold deposits also contain at least one population of high-salinity aqueous brine.Oxygen and hydrogen isotope data for both styles of deposit usually cannot distinguish between a magmatic or metamorphic source for the ore-bearing fluids.However,sulfur and lead isotope data for the intrusion-related gold deposits generally indicate either a magmatic source or mixing between magmatic and sedimentary sources of fluid.The metamorphic geothermal gradients associated with intrusion-related gold deposits are characterized by low pressure,high temperature metamorphism and high crustal geothermal gradients of>30/km.Where amphibole breakdown occurs in a granite source region,the spatially related deposits are more commonly associated with Cu-Au deposits rather than Au-only deposits that are associated with lower temperature granites.The dominant processes thought to cause gold precipitation in both types of deposits are fluid-rock interaction(e.g.desulfidation)or phase separation.Consideration of the physical and chemical properties of the H_2O-NaCl-CO_2 system on the nature of gold precipitation mechanisms at different crustal levels infers different roles of chemical(fluid-rock interaction)versus rheological(phase separation and/or fluid mixing)host-rock controls on gold deposition.This also implies that at the site of deposition,similar precipitation mechanisms operate at similar crustal levels for both orogenic and intrusion-related gold deposits.  相似文献   
96.
岩体在块系构造状态下的动力传播存在块体和块体间软弱介质的非协调变形现象,对岩体结构的动力稳定产生重要影响。目前块系岩体的非协调动力传播响应研究尚不充分,导致不能进行有效的动力响应特征识别。通过试验对块系岩体非协调动力传播过程岩块动力响应特征进行研究,分别从动力传播速度、岩块加速度振幅衰减、岩块振动位移响应、岩块振动持续时间、块体动能显现、块体振动频域响应特性等方面对比纵波传播,给出块系岩体非协调动力传播的特征分析。通过分析可知,块系介质非协调变形运动产生的动力传播现象相比于纵波传播是一种低频低速波,并伴随着岩块的大位移运动,同时岩块振动持续时间较长,蕴含着动能与势能的相互转换过程,这些现象构成了块系岩体非协调动力传播的重要特征。该研究将为识别岩体非协调动力传播特征及块系岩体的冲击预警波动特征识别提供参考。  相似文献   
97.
98.
Morih.  N 《探矿工程译丛》1998,(4):13-14,19
该文描述了旋喷注浆在地下24.8-28.3m深处两条3.5m直径质构隧道连接中的应用。两隧道交接处的地层主要为松散的中细粒砂土,其间夹有一些坚固的细粉砂透镜体和坚硬的砂性土。这些坚硬减小了水射流的作用范围。采用与标准旋喷注浆不同的特殊参数与工艺,这一问题得到了解决使得旋喷桩径达到了1.6m。另外,在完成导向孔钻进后,用测斜仪对其进行了垂直精度测量,以确保注浆固结体的均匀性。两质构隧道以成功地连接。  相似文献   
99.
如果在松软地层上进行建筑施工,必须采取措施,防止横向位移、压密沉陷和由于地层滑移和差异沉降引起的不稳定性。本文首先概要地讨论了利用人造地层加固方法,作为对松软地层采取的措施。其次提出多锚栓墙结合陡坡加固堤岸的预加载施工方法,目的在于减少差异沉降.试验堤坝和实际施工证实方法的实用性和效果。  相似文献   
100.
罗斯基勒(Roskilde)大学(丹麦)开展沿海地区的环境监测已有若干年了,其中包括不久前在波罗地海区与俄罗斯圣彼德堡科学工作者们的一项重要国际合作。起初研究这些方法是为了确定矿物原料在海底的位置,但目前这些方法已完全可用于一般的环境监测。在不久的将来,一些电测方法肯定会有产业性的突破。这种进步好比60年代海洋地震带来的重要突破。电阻率法、电阻抗谱法(EIS)与自然电场法的组合,包括离子选择电极(  相似文献   
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