全文获取类型
收费全文 | 4642篇 |
免费 | 803篇 |
国内免费 | 1176篇 |
专业分类
测绘学 | 2071篇 |
大气科学 | 2107篇 |
地球物理 | 454篇 |
地质学 | 389篇 |
海洋学 | 568篇 |
天文学 | 301篇 |
综合类 | 457篇 |
自然地理 | 274篇 |
出版年
2024年 | 15篇 |
2023年 | 60篇 |
2022年 | 208篇 |
2021年 | 279篇 |
2020年 | 291篇 |
2019年 | 227篇 |
2018年 | 164篇 |
2017年 | 357篇 |
2016年 | 294篇 |
2015年 | 338篇 |
2014年 | 316篇 |
2013年 | 397篇 |
2012年 | 380篇 |
2011年 | 314篇 |
2010年 | 233篇 |
2009年 | 267篇 |
2008年 | 263篇 |
2007年 | 302篇 |
2006年 | 275篇 |
2005年 | 234篇 |
2004年 | 223篇 |
2003年 | 210篇 |
2002年 | 136篇 |
2001年 | 128篇 |
2000年 | 122篇 |
1999年 | 76篇 |
1998年 | 74篇 |
1997年 | 69篇 |
1996年 | 71篇 |
1995年 | 59篇 |
1994年 | 75篇 |
1993年 | 45篇 |
1992年 | 33篇 |
1991年 | 25篇 |
1990年 | 15篇 |
1989年 | 11篇 |
1988年 | 10篇 |
1987年 | 10篇 |
1986年 | 5篇 |
1985年 | 2篇 |
1984年 | 2篇 |
1982年 | 1篇 |
1980年 | 2篇 |
1978年 | 1篇 |
1954年 | 2篇 |
排序方式: 共有6621条查询结果,搜索用时 31 毫秒
71.
多源遥感影像数据的融合方法探讨 总被引:1,自引:0,他引:1
孔庆楠 《测绘与空间地理信息》2008,31(4)
在分析和总结多源遥感影像数据融合的基础上,探讨了多源遥感影像数据融合的层次、模型、结构及其特点.归纳总结了多源遥感影像数据融合方法,目的是提高多光谱影像分辨率的同时保持色调不变,从另一个角度理解为在已知低分辨率多光谱影像和高分辨率全色影像的基础上,模拟生成高分辨率多光谱影像.本文介绍了遥感影像融合技术,系统阐述了几种常见的遥感影像融合方法及其应用. 相似文献
72.
作者探索利用已有的控制点成果及1∶10000地形图矢量数据、高分辨率Quickbird卫星遥感影像,针对国内各省近年更新过的1∶10000数字正射影像数据、1∶10000地形图数据进行再次更新的方法进行了探索。 相似文献
73.
震前卫星热红外环形应力场特征 总被引:6,自引:1,他引:5
本文包括两部分内容:①描述了1996年2月3日云南丽江Ms7.0级地震,震前几天的卫星热红外图像呈现圆形,它的NNW、NW、SN、及NE向的热旋扭面往S收敛。该地震地表破裂由一系列张扭性裂缝组成,呈左旋左列,水平位错不明显,垂直断距数厘米。垂直力对构造变动的作用较为明显;而丽江地震震源机制解破裂面II的走向NNE6o,倾向W,倾角44o,P轴方位为NNE3o、仰角75o,近于直立,综合热旋扭面展布、地震地表破裂特征及震源机制解,得出该旋扭椭圆为地幔外侧右旋上涌所造成;②菲律宾萨马岛Ms7.0~7.5强震群及青海共和Ms7.0地震前热应力环椭圆的推进路径。根据这一特征得出交变潮汐力的地球动力学解释。卫星热红外图像震前应力热场的方法是临震预测地震的有效方法,卫星热红外技术辅以震源机制解和地表破裂带力学分析是研究地球动力学有力工具。地球自转速度变化,交变潮汐力和地幔旋扭上涌力是地球动力学的主因。 相似文献
74.
75.
The dynamics and thermodynamics of large ash flows 总被引:6,自引:6,他引:0
Ash flow deposits, containing up to 1000 km3 of material, have been produced by some of the largest volcanic eruptions known. Ash flows propagate several tens of kilometres
from their source vents, produce extensive blankets of ash and are able to surmount topographic barriers hundreds of metres
high. We present and test a new model of the motion of such flows as they propagate over a near horizontal surface from a
collapsing fountain above a volcanic vent. The model predicts that for a given eruption rate, either a slow (10–100 m/s) and
deep (1000–3000 m) subcritical flow or a fast (100–200 m/s) and shallow (500–1000 m) supercritical flow may develop. Subcritical
ash flows propagate with a nearly constant volume flux, whereas supercritical flows entrain air and become progressively more
voluminous. The run-out distance of such ash flows is controlled largely by the mass of air mixed into the collapsing fountain,
the degree of fragmentation and the associated rate of loss of material into an underlying concentrated depositional system,
and the mass eruption rate. However, in supercritical flows, the continued entrainment of air exerts a further important control
on the flow evolution. Model predictions show that the run-out distance decreases with the mass of air entrained into the
flow. Also, the mass of ash which may ascend from the flow into a buoyant coignimbrite cloud increases as more air is entrained
into the flow. As a result, supercritical ash flows typically have shorter runout distances and more ash is elutriated into
the associated coignimbrite eruption columns. We also show that one-dimensional, channellized ash flows typically propagate
further than their radially spreading counterparts.
As a Plinian eruption proceeds, the erupted mass flux often increases, leading to column collapse and the formation of pumiceous
ash flows. Near the critical conditions for eruption column collapse, the flows are shed from high fountains which entrain
large quantities of air per unit mass. Our model suggests that this will lead to relatively short ash flows with much of the
erupted material being elutriated into the coignimbrite column. However, if the mass flux subseqently increases, then less
air per unit mass is entrained into the collapsing fountain, and progressively larger flows, which propagate further from
the vent, will develop.
Our model is consistent with observations of a number of pyroclastic flow deposits, including the 1912 eruption of Katmai
and the 1991 eruption of Pinatubo. The model suggests that many extensive flow sheets were emplaced from eruptions with mass
fluxes of 109–1010 kg/s over periods of 103–105 s, and that some indicators of flow "mobility" may need to be reinterpreted. Furthermore, in accordance with observations,
the model predicts that the coignimbrite eruption columns produced from such ash flows rose between 20 and 40 km.
Received: 25 August 1995 / Accepted: 3 April 1996 相似文献
76.
The Bureau of Economic Analysis (BEA), U.S. Department of Commerce, in keeping with broad international efforts to green national gross domestic product (GDP) accounts, has attempted to create satellite accounts for mineral depletion. The present paper criticizes the BEA's unit rent measure of resource depletion, which is based upon Hotelling's pure theory of exhaustion. Following a thorough criticism of Hotelling's theory as a real-world model of mineral prices, practical issues related to the treatment of recycling, exploration, definition of reserves/resources, and their valuation/exploitation are introduced. For crude oil and natural gas and the nonfuel minerals, specific application problems of joint products and residuals complicate BEA's assumptions and efforts. 相似文献
77.
D. Rouan N. Epchtein M. De Muizon F. Lacombe P. Puget D. Tiphene F. Boulanger X. Desert G. Guyot L. D'Hendecourt J -M. Lamarre A. Leger F. Pajot J -L. Puget E. Caux M. Giard G. Serra C. Cesarsky L. Vigroux A. Omont 《Astrophysics and Space Science》1994,217(1-2):41-44
Proposed to both the French and the European Space Agency as one possible small mission, SPICE is a project for a dedicated small satellite for a near-IR spectroscopic all-sky survey. The instrument would cover the spectral range 1.8 - 3.6µm, possibly extended to 1.8 - 7µm, at a resolution of 100, with pixels of 1 arc-min. The excellent sensitivity (0.02 MJy sr-1) results from: i) the quasi-zero level of background due to the efficient passive cooling of the whole experiment; ii) the use of large format arrays; iii) the non-stop observing mode (drift-scanning). The spectral domain, complementing the one of ISO, partially opaque from the ground, is specially rich in spectral features tracing stars and all components of the Interstellar Medium (molecular, atomic and ionized gas, dust). With a cooling below 80 K of the focal instrument, then it becomes possible to consider doubling the spectral domain and to cover the whole 1.8 - 7µm range. 相似文献
78.
我国风云极轨气象卫星数据,目前已经被应用在天气预报、气候预测、自然灾害、环境监测、科学研究等多个重要领域,为我国国民经济建设、国防建设、防灾减灾和全球许多国家的经济发展做出了重要贡献。本文介绍了我国风云极轨气象卫星的发展历程,重点阐述了目前风云极轨气象卫星在卫星数据预处理、定量产品反演、卫星资料同化等方面的应用研究进展,并展示了第二代风云极轨气象卫星在全球业务观测、大气三维探测、海洋环境监测、数值预报应用等相关典型应用。在国家创新战略发展框架下,根据“国家级气象现代化总体方案”确定的2020年气象卫星及应用发展目标,第二代极轨气象卫星风云三号03批卫星系统工程必将进一步发挥重大支撑作用。 相似文献
79.
A. G. Mavraganis 《Celestial Mechanics and Dynamical Astronomy》1991,51(4):395-405
The almost constant-speed motion of a mass acted upon by a Newtonian attraction and a resisting force is treated. The equation of orbit is derived for a specific type of resistance which covers the familiar case of Danby's drag(=r
–2) whilst the vector invariants are obtained by direct operation on the vector form of the equation of motion. 相似文献
80.
Cloud droplet chemistry is modelled for the first 150 m of rise in a wintertime, mid-latitude, marine stratus cloud using observations made at and near the Cape Grim Baseline Station as a source of input parameters. The emphasis in this work was to study the variation in droplet chemistry as a function of both droplet size and nucleus composition, with a particular focus on the way in which oxidation of dissolved sulfur dioxide varied.At 150 m above the condensation level, solute concentration as a function of droplet size was found to increase by as much as 2 to 3 orders of magnitude for only a factor of 2 increase in droplet radius, primarily as a consequence of the 1/r dependence in the droplet growth equation. This type of size dependence exists at all levels in the model cloud, and has a significant influence on oxidation rate of sulfur dioxide in droplets growing on sulfate nuclei, oxidation by ozone being favoured in the smallest droplets, but oxidation by hydrogen peroxide being favoured in the larger droplets. Oxidation by ozone is favoured at all sizes in droplets formed on sea-salt nuclei as a result of the initially high alkalinity of these droplets, and in the cloud overall is calculated to be the more important oxidation pathway. Although based on a simplified chemical scheme, these results suggest that both size-dependent and nucleus-dependent chemistry of cloud droplets may need to be considered explicitly in cloud modelling work.Volume-weighted mean pH values in the range 5 to 6 were predicted from sensitivity studies in which input variables were varied over reasonable ranges, in agreement with two sets of bulk cloud-water pH data obtained by aircraft near Cape Grim. 相似文献