全文获取类型
收费全文 | 8566篇 |
免费 | 789篇 |
国内免费 | 899篇 |
专业分类
测绘学 | 4174篇 |
大气科学 | 680篇 |
地球物理 | 818篇 |
地质学 | 2408篇 |
海洋学 | 631篇 |
天文学 | 278篇 |
综合类 | 535篇 |
自然地理 | 730篇 |
出版年
2024年 | 17篇 |
2023年 | 63篇 |
2022年 | 201篇 |
2021年 | 244篇 |
2020年 | 285篇 |
2019年 | 390篇 |
2018年 | 196篇 |
2017年 | 387篇 |
2016年 | 387篇 |
2015年 | 424篇 |
2014年 | 466篇 |
2013年 | 551篇 |
2012年 | 528篇 |
2011年 | 555篇 |
2010年 | 414篇 |
2009年 | 477篇 |
2008年 | 502篇 |
2007年 | 526篇 |
2006年 | 492篇 |
2005年 | 471篇 |
2004年 | 403篇 |
2003年 | 364篇 |
2002年 | 282篇 |
2001年 | 271篇 |
2000年 | 214篇 |
1999年 | 192篇 |
1998年 | 200篇 |
1997年 | 155篇 |
1996年 | 119篇 |
1995年 | 102篇 |
1994年 | 75篇 |
1993年 | 79篇 |
1992年 | 59篇 |
1991年 | 44篇 |
1990年 | 34篇 |
1989年 | 27篇 |
1988年 | 20篇 |
1987年 | 16篇 |
1986年 | 12篇 |
1985年 | 1篇 |
1984年 | 1篇 |
1982年 | 4篇 |
1978年 | 2篇 |
1977年 | 1篇 |
1954年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 78 毫秒
991.
Robert I. Reid 《Monthly notices of the Royal Astronomical Society》2006,367(4):1766-1780
A new technique is presented for producing images from interferometric data. The method, 'smear fitting', makes the constraints necessary for interferometric imaging double as a model, with uncertainties, of the sky brightness distribution. It does this by modelling the sky with a set of functions and then convolving each component with its own elliptical Gaussian to account for the uncertainty in its shape and location that arises from noise. This yields much sharper resolution than clean for significantly detected features, without sacrificing any sensitivity. Using appropriate functional forms for the components provides both a scientifically interesting model and imaging constraints that tend to be better than those used by traditional deconvolution methods. This allows it to avoid the most serious problems that limit the imaging quality of those methods. Comparisons of smear fitting to clean and maximum entropy are given, using both real and simulated observations. It is also shown that the famous Rayleigh criterion (resolution = wavelength/baseline) is inappropriate for interferometers as it does not consider the reliability of the measurements. 相似文献
992.
图像减影技术在自动报靶系统中的应用 总被引:3,自引:0,他引:3
袁莉茹 《成都信息工程学院学报》2006,21(3):370-372
弹点分割一直是自动报靶系统的关健技术之一,所提出的减影技术不仅方法简单,而且能大大简化弹点的分割过程,使系统的工作效率明显地提高. 相似文献
993.
利用小波变换进行遥感多光谱图像融合的算法及实现 总被引:3,自引:0,他引:3
在分析了小波变换的分解与重建方法后,提出了一种基于区域的图像增强算法。先提取出源图的边缘,以图像的边缘为参考,围绕边缘建立融合窗口,然后结合区域内的图像信息,应用基于窗口的融合规则进行融合处理。实验结果显示,融合后的图像综合了3幅源图像的不同特征,处理后的图像变得容易识别了。表明该方法保持了尽可能多的原始信息,算法简单,稳定性好,适合于多光谱遥感图像识别、医学成像等领域。 相似文献
994.
995.
Using the Very Large Array (VLA), we observed all three of the 6-cm lines of the 2 Π1/2 , J = 1/2 state of OH with sub-arcsecond resolution (∼0.4 arcsec) in W49A. While the spatial distribution and the range in velocities of the 6-cm lines are similar to those of the ground-state (18-cm) OH lines, a large fraction of the total emission in all three 6-cm lines has large linewidths (∼5–10 km s−1 ) and is spatially extended, very unlike typical ground-state OH masers, which typically are point-like at VLA resolutions and have linewidths ≤1 km s−1 . We find brightness temperatures of 5900, 4700 and ≥730 K for the 4660, 4750 and 4765-MHz lines, respectively. We conclude that these are indeed maser lines. However, the gains are ∼0.3, again very unlike the 18-cm lines, which have gains ≥104 . We compare the excited-state OH emission with that from other molecules observed with comparable angular resolution to estimate physical conditions in the regions emitting the peculiar, low-gain maser lines. We also comment on the relationship with the 18-cm masers. 相似文献
996.
Optimal orbits for Mars atmosphere remote sensing 总被引:1,自引:0,他引:1
Most of the spacecrafts currently around Mars (or planned to reach Mars in the near future) use Sun-synchronous or near-polar orbits. Such orbits offer a very poor sampling of the diurnal cycle. Yet, sampling the diurnal cycle is of key importance to study Mars meteorology and climate. A comprehensive remote sensing data set should have been obtained by the end of the MRO mission, launched in 2005. For later windows, time-varying phenomena should be given the highest priority for remote sensing investigations. We present possible orbits for such missions which provide a rich spatial and temporal sampling with a relatively short repeat cycle (50 sols). After computation and determination of these orbits, said “optimal orbits”, we illustrate our results by tables of sampling and comparison with other orbits. 相似文献
997.
Q. Y. Peng 《Monthly notices of the Royal Astronomical Society》2005,359(4):1597-1600
The image-processing techniques used by Peng et al. are further improved to measure precisely the positions of Saturn and its satellites. 495 CCD images taken with the 1-m telescope at the Yunnan Observatory during the years 2002–2004 are processed with these techniques. These measured pixel positions are compared to their theoretical positions computed with the ephemerides of TASS1.7 for the satellites and JPL DE405 for Saturn itself. Analysis of the data for the intersatellite positions among four bright Saturnian satellites (S3–S6) and for Saturn–satellite (i.e. Saturn–Titan) positions shows that these measured positions have the same dispersions, i.e. about 0.05 and 0.06 arcsec in right ascension and declination, respectively. However, for the fainter satellites, Enceladus and Mimas, poorer residuals up to 0.1 and 0.2 arcsec, respectively, in both directions are found mainly due to their small separations from the primary planet and short exposure time in order to obtain useful images of Saturn. 相似文献
998.
高挂山—牛头寨地区,通过大比例尺航片解译,发现6个大小不等的小型环形影象信息。这些环形影象与岩浆活动、已知矿床、矿化点、重砂异常、物化探异常等的分布有着内在的联系。为预测找矿远景区和找隐伏矿床提供了影象依据。 相似文献
999.
Remote sensing is a geographic analysis tool capable of producing large quantities of data in the spectral, temporal and spatial domains. Techniques for automating the image analysis process would be advanced by the inclusion of artificial intelligence techniques in the design of image processing systems. The remote sensing application which show promise for successful implementation of artificial intelligence techniques are intelligent onboard processing, advanced database interrogation, and the automated analysis of multispectral imagery. 相似文献
1000.
Topography and morphodynamics in the German Bight using SAR and optical remote sensing data 总被引:3,自引:0,他引:3
Morphological changes in coastal areas, especially in river estuaries, are of high interest in many parts of the world. Satellite
data from both optical and radar sensors can help to monitor and investigate these changes. Data from both kinds of sensors
being available for up to 30 years now, allow examinations over large timescales, while high resolution sensors developed
within the last decade allow increased accuracy. So the creation of digital elevation models (DEMs) of, for example, the wadden
sea from a series of satellite images is already possible. ENVISAT, successfully launched on March 1, 2002, continues the
line of higher resolution synthetic aperture radar (SAR) imaging sensors with its ASAR instrument and now also allows several
polarization modes for better separation of land and water areas. This article gives an overview of sensors and algorithms
for waterline determination as well as several applications. Both optical and SAR images are considered. Applications include
morphodynamic monitoring studies and DEM generation.
相似文献
Andreas NiedermeierEmail: |