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通过野外地质调查结合大地电磁测深综合构造解释,在休宁—歙县金多金属矿整装勘查区及邻区厘定出发育于晚侏罗世的较大规模逆冲推覆构造,其由逆冲断层、逆冲岩席、原地岩系、构造窗及伴生的牵引褶皱等组成。该逆冲推覆构造发育于"屯溪—休宁"红层盆地南缘,表现为晚元古代浅变质火山-碎屑岩系逆冲推覆于中侏罗统洪琴组碎屑岩之上。逆冲推覆构造由一系列分支逆断层组成,以前展式叠瓦状逆冲为特征,断层前缘陡立,向下变缓。逆冲推覆构造呈北东走向展布,勘查区内延伸可达40 km,推覆体面积大于600 km2。构造窗出露位置结合钻探、物探揭示,逆冲位移为2.0~8.0 km。根据逆冲断层时空配套以及岩浆活动与波及的沉积地层,判断晚侏罗世逆冲推覆构造活动时间为163.5~149.0 Ma。通过逆冲断层擦痕观察及古应力场分析,认为该期逆冲推覆构造形成于华南板块向北强烈挤压的区域动力学环境。逆冲推覆构造为成矿前构造,其与之后发生的伸展构造对岩浆的侵入及含矿热液的流通起着重要的作用,控制了整装勘查区内金、银、铅锌等中低温元素的分布与富集成矿。 相似文献
113.
Urban heat island monitoring and analysis using a non-parametric model: A case study of Indianapolis 总被引:1,自引:0,他引:1
Umamaheshwaran Rajasekar Qihao Weng 《ISPRS Journal of Photogrammetry and Remote Sensing》2009,64(1):86-96
A procedure for the monitoring an urban heat island (UHI) was developed and tested over a selected location in the Midwestern United States. Nine counties in central Indiana were selected and their UHI patterns were modeled. Moderate Resolution Imaging Spectroradiometer (MODIS) land surface temperature (LST) images taken in 2005 were used for the research. The images were sorted based on cloud cover over the study area. The resulting 94 day and night images were used for the modeling. The technique of process convolution was then applied to the images in order to characterize the UHIs. This process helped to characterize the LST data into a continuous surface and the UHI data into a series of Gaussian functions. The diurnal temperature profiles and UHI intensity attributes (minimum, maximum and magnitude) of the characterized images were analyzed for variations. Skin temperatures within any given image varied between 2–15 °C and 2–8 °C for the day and night images, respectively. The magnitude of the UHI varied from 1–5 °C and 1–3 °C over the daytime and nighttime images, respectively. Three dimensional (3-D) models of the day and night images were generated and visually explored for patterns through animation. A strong and clearly evident UHI was identified extending north of Marion County well into Hamilton County. This information coincides with the development and expansion of northern Marion County during the past few years in contrast to the southern part. To further explore these results, an Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) 2004 land use land cover (LULC) dataset was analyzed with respect to the characterized UHI. The areas with maximum heat signatures were found to have a strong correlation with impervious surfaces. The entire process of information extraction was automated in order to facilitate the mining of UHI patterns at a global scale. This research has proved to be promising approach for the modeling and mining of UHIs from large amount of remote sensing images. Furthermore, this research also aids in 3-D diachronic analysis. 相似文献
114.
Case-based reasoning is an AI technique in which the previous solutions are stored for future use. People are used to guiding themselves according to those routes that are stored in their memories and have been used by them before. It is just based on people’s preference to familiar routes, which are gained through the study of the cognitive activities. We propose to apply the intelligent method based on the case reasoning to path planning. It is impossible for a case base to store all the solutions to all the shortest paths; therefore, part of them should be stored. However, which routes should be stored and which should not be? How do we adapt the cases that have already been stored and how do we acquire the shortest route based on them? All these issues need to be explained by integrating knowledge of the network on account of case-based reasoning techniques. This paper suggests the case-based reasoning in another point. This means finding some irreplaceable links on the basis of the complete analysis of the problems space, which are called the must_be_passed link between the source and destination. Merely compute the shortest path case from those best exit/entry nodes of the grids to the irreplaceable links, and then add them into the case base storing for future use. This method is based on case-based reasoning technique and completely considers the properties of the problem space. In addition to the use of knowledge of the natural grid in the route network, this method is more efficient than existing algorithms on computing efficiency. 相似文献
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热带西太平洋暖池是全球大洋表面温度最高的区域,也是全球海-气能量交换年总量最大的海域。它的维持和变化不仅对El Nifio的发生、发展起着重要作用,而且对中高纬度大气环流的变化也有重要影响。近年来国内外对热带西太平洋暖池进行了许多实验和研究,取得了一些有意义的结果(王世平,1989; Wyrtki,1989;黄荣辉,1994;董敏,1994;Wajsowicz,1994)。但是这些研究多偏重于暖池对大气环流和东亚气候的影响方面,对暖池本身的主要特征及其变异方面的研究相对较少,而后者却是进一步了解发生在暖池区的海-气相互作用的过程,研究暖池在全球气候变化中的作用所不可缺少的。本文在分析1951-1990年间的SST资料和137°E,155°E,165°E断面观测结果的基础上,结合有关研究成果(符淙斌,1990),对暖池的形态、高温中心和热含量这三个主要特征及其变异特点进行了研究,并初步找出了暖池表面面积与南方涛动指数和副热带高压面积指数间的关系。 相似文献
117.
Peter A. Taylor P-Y. Li Diane V. Michelangeli Jagruti Pathak Wensong Weng 《Boundary-Layer Meteorology》2007,125(2):305-328
A time and height dependent eddy diffusion model is used to investigate possible scenarios for the size distribution of dust
in the lower atmosphere of Mars. The dust is assumed to either have been advected from a distant source or to have originated
locally. In the former case, the atmosphere is assumed to initially contain dust particles with sizes following a modified
gamma distribution. Larger particles are deposited relatively rapidly while small particles are well mixed up to the maximum
height of the afternoon boundary layer and are deposited more slowly. In other cases, a parameterization of the dust source
at the surface is proposed. Model results show that smaller particles are rapidly mixed within the Martian boundary layer,
while larger particles (r > 10 μm) are concentrated near the ground with a stronger diurnal cycle. In all simulations we assume
that the initial concentration or surface source depend on a modified gamma function distribution. For small particles (cross-
sectional area weighted mean radius, reff = 1.6 μm) distributions retain essentially the same form, though with variations in the mean and variance of the area-weighted
radius, and the gamma function can be used to represent the particle size distribution reasonably well at most heights within
the boundary layer. In the case of a surface source of larger particles (mean radius 50 μm) the modified gamma function does
not fit the resulting particle size distribution. All results are normalised by a scaling factor that can be adjusted to correspond
to an optical depth for assumed particle optical scattering properties. 相似文献
118.
利用2003年10月北京地区PM10浓度流动观测资料和同期MODIS AOD(Aerosol Optical Depth)高分辨率遥感资料,采用卫星遥感地面观测变分订正处理方法,综合分析了北京地区PM10浓度的空间分布特征以及机动车排放的影响效应。动态观测试验结果表明:北京城区大部分为轻污染区, 北京近郊区PM10浓度高值区沿环路呈环状分布,其中北京西南部、南部和东北部污染较严重,北京城郊街区PM10的空间分布受机动车排放的影响较大。MODIS卫星遥感资料分析表明:北京城区及近郊区AOD值较远郊区高得多,AOD空间分布场中存在虚假高值区,AOD非均匀分布特征不明显。采取点面结合综合观测研究思路,运用卫星遥感地面观测综合变分分析方法,可以取得客观订正的显著效果。经地面实测PM10浓度变分订正后的AOD变分场可以较高分辨率信息描述北京地区AOD的非均匀分布特征,弥补地面PM10浓度观测的缺陷。 相似文献
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