全文获取类型
收费全文 | 2984篇 |
免费 | 301篇 |
国内免费 | 584篇 |
专业分类
测绘学 | 675篇 |
大气科学 | 594篇 |
地球物理 | 484篇 |
地质学 | 1098篇 |
海洋学 | 245篇 |
天文学 | 183篇 |
综合类 | 213篇 |
自然地理 | 377篇 |
出版年
2024年 | 15篇 |
2023年 | 28篇 |
2022年 | 58篇 |
2021年 | 97篇 |
2020年 | 102篇 |
2019年 | 112篇 |
2018年 | 65篇 |
2017年 | 109篇 |
2016年 | 121篇 |
2015年 | 123篇 |
2014年 | 147篇 |
2013年 | 186篇 |
2012年 | 157篇 |
2011年 | 206篇 |
2010年 | 136篇 |
2009年 | 158篇 |
2008年 | 212篇 |
2007年 | 212篇 |
2006年 | 218篇 |
2005年 | 184篇 |
2004年 | 136篇 |
2003年 | 159篇 |
2002年 | 142篇 |
2001年 | 102篇 |
2000年 | 110篇 |
1999年 | 90篇 |
1998年 | 84篇 |
1997年 | 61篇 |
1996年 | 67篇 |
1995年 | 60篇 |
1994年 | 62篇 |
1993年 | 31篇 |
1992年 | 34篇 |
1991年 | 33篇 |
1990年 | 16篇 |
1989年 | 12篇 |
1988年 | 9篇 |
1987年 | 2篇 |
1986年 | 2篇 |
1985年 | 3篇 |
1983年 | 1篇 |
1980年 | 1篇 |
1979年 | 1篇 |
1978年 | 2篇 |
1976年 | 1篇 |
1954年 | 2篇 |
排序方式: 共有3869条查询结果,搜索用时 15 毫秒
371.
Tele-connecting local consumption to global land use 总被引:1,自引:0,他引:1
Globalization increases the interconnectedness of people and places around the world. In a connected world, goods and services consumed in one country are often produced in other countries and exchanged via international trade. Thus, local consumption is increasingly met by global supply chains oftentimes involving large geographical distances and leading to global environmental change. In this study, we connect local consumption to global land use through tracking global commodity and value chains via international trade flows. Using a global multiregional input–output model with sectoral detail allows for the accounting of land use attributed to “unusual” sectors – from a land use perspective – including services, machinery and equipment, and construction. Our results show how developed countries consume a large amount of goods and services from both domestic and international markets, and thus impose pressure not only on their domestic land resources, but also displace land in other countries, thus displacing other uses. For example, 33% of total U.S. land use for consumption purposes is displaced from other countries. This ratio becomes much larger for the EU (more than 50%) and Japan (92%). Our analysis shows that 47% of Brazilian and 88% of Argentinean cropland is used for consumption purposes outside of their territories, mainly in EU countries and China. In addition, consumers in rich countries tend to displace land by consuming non-agricultural products, such as services, clothing and household appliances, which account for more than 50% of their total land displacement. By contrast, for developing economies, such as African countries, the share of land use for non-agricultural products is much lower, with an average of 7%. The emerging economies and population giants, China and India, are likely to further increase their appetite for land from other countries, such as Africa, Russia and Latin America, to satisfy their own land needs driven by their fast economic growth and the needs and lifestyles of their growing populations. 相似文献
372.
Abstract The purpose of this article is to analyse whether the presence of surplus emission allowance trading jeopardizes the environmental target of an international environmental agreement. We argue that surplus emission allowance trading can be used as an implicit side-payment mechanism to actually bring about higher environmental protection compared with the situation without the trade option. We point to the existence of a fundamental trade-off between costs of compliance and the creation of dynamic incentives to develop cheaper reduction technologies. Implicit side payments, in terms of surplus emission allocations, may be needed in order to establish a compromise between these opposing demands. We identify the shortcomings and benefits of allowing fully flexible permit trading, including the allocation rule of grandfathering. 相似文献
373.
基于通信卫星的导航系统可以利用比地球静止轨道(Geostationary Earth Orbit,GEO)高约200 km的倾斜高圆轨道(inclined Highly Circular Orbit,iHCO)通信卫星组成导航星座.结合两种轨道高度的倾斜高圆轨道通信卫星,仿真分析了利用倾斜高圆轨道卫星组成的中国区域定位系统(Chinese Area Positioning System,CAPS)的导航性能,并讨论了利用倾斜高圆轨道卫星组成的中国区域定位系统实现中国区域覆盖的最佳星座布局. 相似文献
374.
在中国区域定位系统(Chinese Area Positioning System,CAPS)中,带通滤波器是用户接收机的重要组成部分,对于宽频测距码来说,其群时延特性是测距的重要误差来源之一.分析了接收机码跟踪环路,给出相关函数估算测距偏差,对带通滤波器群时延开展仿真分析,并研究了改进接收机设计以优化群时延特性的方法.研究对GNSS接收机的射频和环路设计有一定借鉴意义. 相似文献
375.
376.
Connecting atmospheric science and atmospheric models for aerocapture at Titan and the outer planets
Many atmospheric measurement systems, such as the sounding instruments on Voyager, gather atmospheric information in the form of temperature versus pressure level. In these terms, there is considerable consistency among the mean atmospheric profiles of the outer planets Jupiter through Neptune, including Titan. On a given planet or on Titan, the range of variability of temperature versus pressure level due to seasonal, latitudinal, and diurnal variations is also not large. However, many engineering needs for atmospheric models relate not to temperature versus pressure level but atmospheric density versus geometric altitude. This need is especially true for design and analysis of aerocapture systems. Drag force available for aerocapture is directly proportional to atmospheric density. Available aerocapture “corridor width” (allowable range of atmospheric entry angle) also depends on height rate of change of atmospheric density, as characterized by density scale height. Characteristics of hydrostatics and the gas law equation mean that relatively small systematic differences in temperature versus pressure profiles can integrate at high altitudes to very large differences in density versus altitude profiles. Thus, a given periapsis density required to accomplish successful aerocapture can occur at substantially different altitudes (∼150-300 km) on the various outer planets, and significantly different density scale heights (∼20-50 km) can occur at these periapsis altitudes. This paper will illustrate these effects and discuss implications for improvements in atmospheric measurements to yield significant impact on design of aerocapture systems for future missions to Titan and the outer planets. Relatively small-scale atmospheric perturbations, such as gravity waves, tides, and other atmospheric variations can also have significant effect on design details for aerocapture guidance and control systems. This paper will discuss benefits that would result from improved understanding of Titan and outer planetary atmospheric perturbation characteristics. Details of recent engineering-level atmospheric models for Titan and Neptune will be presented, and effects of present and future levels of atmospheric uncertainty and variability characteristics will be examined. 相似文献
377.
城市规划信息系统作为城市地理信息系统的一个重要的专题分支系统 ,是城市规划体系的基础和纽带。因此 ,通过研究城市规划信息系统的基础理论来指导城市规划信息系统的具体实践 ,进而实现城市可持续发展的战略 ,具有重要意义。 相似文献
378.
1997年11月14日晚,在中国科学院云南天文台1米望远镜上用新安装的10242CCD观测到了木星的两颗伽里略卫星;Europa和Callisto及一颗依巴谷星(星号为 104297).当采用新的 JPL DE405和 Sampson-Lieske理论(G5)计算卫星的理论位置并相对于Callisto测量恒星位置时,视位置的观测值与计算值之差的平均值在赤经和赤纬方向分别为△α=-0″029±0.″012,△δ=0.″005± 0.″011.这对应于平均观测历元(UT):1997年11月14日13时43分50秒.这一试验结果与 Casas等在同一时期内CCD观测的结果有着很好的一致性 它反映了依巴谷星表体现的光学参考系与DE405体现的动力学参考系在观测历元具有较好的一致性.单次位置测定的标准误差在赤经赤纬方向分别为±0.″052和0.″047.这一精度明显优于 Casas等人发表的 Callisto的处理精度,并与目前国际上最好的伽里略卫星观测精度相当 相似文献
379.
Ca-Al rich refractory mineral inclusions (CAIs) found at 1-6% mass fraction in primitive chondrites appear to be 1-3 million years older than the dominant (chondrule) components which were accreted into the same parent bodies. A prevalent concern is that it is difficult to retain CAIs for this long against gas-drag-induced radial drift into the Sun. We reassess the situation in terms of a hot inner (turbulent) nebula context for CAI formation, using analytical models of nebula evolution and particle diffusion. We show that outward radial diffusion in a weakly turbulent nebula can overcome inward drift, and prevent significant numbers of CAI-size particles from being lost into the Sun for times on the order of 106 years. CAIs can form early, when the inner nebula was hot, and persist in sufficient abundance to be incorporated into primitive planetesimals at a much later time. Small (?0.1 mm diameter) CAIs persist for longer times than large (?5 mm diameter) ones. To obtain a quantitative match to the observed volume fractions of CAIs in chondrites, another process must be allowed for: a substantial enhancement of the inner hot nebula in silicate-forming material, which we suggest was caused by rapid inward drift of meter-sized objects. This early in nebula history, the drifting rubble would have a carbon content probably an order of magnitude larger than even the most primitive (CI) carbonaceous chondrites. Abundant carbon in the evaporating material would help keep the nebula oxygen fugacity low, plausibly solar, as inferred for the formation environment of CAIs. The associated production of a larger than canonical amount of CO2 might also play a role in mass-independent fractionation of oxygen isotopes, leaving the gas rich in 16O as inferred from CAIs and other high temperature condensates. 相似文献