全文获取类型
收费全文 | 3169篇 |
免费 | 334篇 |
国内免费 | 482篇 |
专业分类
测绘学 | 1242篇 |
大气科学 | 548篇 |
地球物理 | 425篇 |
地质学 | 822篇 |
海洋学 | 368篇 |
天文学 | 76篇 |
综合类 | 328篇 |
自然地理 | 176篇 |
出版年
2024年 | 3篇 |
2023年 | 22篇 |
2022年 | 49篇 |
2021年 | 82篇 |
2020年 | 105篇 |
2019年 | 104篇 |
2018年 | 76篇 |
2017年 | 126篇 |
2016年 | 143篇 |
2015年 | 157篇 |
2014年 | 180篇 |
2013年 | 212篇 |
2012年 | 196篇 |
2011年 | 237篇 |
2010年 | 168篇 |
2009年 | 192篇 |
2008年 | 199篇 |
2007年 | 220篇 |
2006年 | 216篇 |
2005年 | 178篇 |
2004年 | 143篇 |
2003年 | 110篇 |
2002年 | 103篇 |
2001年 | 87篇 |
2000年 | 77篇 |
1999年 | 73篇 |
1998年 | 100篇 |
1997年 | 64篇 |
1996年 | 57篇 |
1995年 | 43篇 |
1994年 | 43篇 |
1993年 | 42篇 |
1992年 | 35篇 |
1991年 | 31篇 |
1990年 | 26篇 |
1989年 | 33篇 |
1988年 | 13篇 |
1987年 | 13篇 |
1986年 | 10篇 |
1985年 | 5篇 |
1984年 | 7篇 |
1982年 | 2篇 |
1981年 | 1篇 |
1980年 | 1篇 |
1954年 | 1篇 |
排序方式: 共有3985条查询结果,搜索用时 15 毫秒
1.
初轨计算中的病态分析 总被引:5,自引:0,他引:5
本文对现有初轨计算方法进行病态性分析与误差分析;研究结果表明:病态对现有初轨算法的影响,主要来源于法方程系数中包含观测误差.系数行列式愈大,定轨精度的损失愈多,当■被随机误差项△μ淹盖时,现有初轨算法将失效.此外,仿真结果还显示:■与△μ的大小还极大地依赖观测弧段的空间位置,当观测弧段包含近站点作为中点时,■最大,而■小,此时定轨精度较高;当观测弧段位于近站点的某一侧时,■小,而■大,此时定轨精度较低,观测弧段愈偏离近站点,病态影响愈大;因而在观测时,应尽量使观测弧段与近站点对称(此时μ值较大),这是提高短弧定轨的一种有效途径. 相似文献
2.
对于改进的Encke方法,选择适当的参考轨道是一个关键.然而,对于人造地球卫星长弧轨道计算,目前所给出的几种参考轨道均需要逐段校正,这将给定轨问题带来附加的复杂性.本文将仔细探讨如何选择参考轨道和减少校正次数. 相似文献
3.
在GPS数据处理中 ,存在着误差影响、影响波的干扰、周跳和数据量大等问题。误差影响和影响波的干扰实质是在接收卫星信号时受到其它因素的影响 ;周跳是由于卫星信号的失锁而造成信号的不连续 ;数据量大是因为GPS观测需要采样间隔小又连续观测所致。由于小波理论具有时频分析、波形分解、特征提取和快速小波变换等特性 ,应用小波变换和波形分解可以解决误差影响和影响波的干扰的问题 ;应用特征提取可以解决周跳检测问题 ;应用快速小波变换可进行数据压缩 相似文献
4.
韩玲 《地球科学与环境学报》2003,25(1):74-75
提出了一种基于格网DEM的粗差检测及剔除方法,其基本思想是对每个表面上的点,在坡度上,高程或突变量引起的形状不连续,可能被怀疑有误差,通过坡度上每个点,应用坡度逼近或改变量来计算,考虑坡度变化的相对值,并以这些相对值计算一个统计值为判断该点合法性的阈值,使计算结果更为可靠。 相似文献
5.
Synthetic SH seismograms in a laterally varying medium by the discrete wavenumber method 总被引:1,自引:0,他引:1
Summary. We present a new method to calculate the SH wavefield produced by a seismic source in a half-space with an irregular buried interface. The diffracting interface is represented by a distribution of body forces. The Green's functions needed to solve the boundary conditions are evaluated using the discrete wavenumber method. Our approach relies on the introduction of a periodicity in the source-medium configuration and on the discretization of the interface at regular spacing. The technique developed is applicable to boundaries of arbitrary shapes and is valid at all frequencies. Some examples of calculation in simple configurations are presented showing the capabilities of the method. 相似文献
6.
提要 本文详细讨论了一种三维重力位场快速正反演方法。作者在前人工作的基础上,对算法作了行之有效的改进,通过对反演中的不稳定因素进行各种理论模型试算,得出保证迭代反演稳定收敛的准则,编制出可在微型机IBM—PC上运行的人机对话式自动正反演程序。本文还对各种不均质模型进行了模似计算并将该方法应用于某含油气沉积盆地的双层界面构造研究,揭示出了储油有利地段。 相似文献
7.
林菁 《广东海洋大学学报》1996,(1)
分析了分频和CTC计数采样中误读数的原因和解决方法,并利用微机软件实现非线性校正。此传感器用于位移测量系统中,具有0.01mm的分辨率及优于1%的精度,可在-20~60℃温度范围内工作。 相似文献
8.
Yu. G. Shkuratov K. Muinonen E. Bowell K. Lumme J. I. Peltoniemi M. A. Kreslavsky D. G. Stankevich V. P. Tishkovetz N. V. Opanasenko L. Y. Melkumova 《Earth, Moon, and Planets》1994,65(3):201-246
About a dozen physical mechanisms and models aspire to explain the negative polarization of light scattered by atmosphereless celestial bodies. This is too large a number for the reliable interpretation of observational data. Through a comparative analysis of the models, our main goal is to answer the question: Does any one model have an advantage over the others? Our analysis is based on new laboratory polarimetric and photometric data as well as on theoretical results. We show that the widely used models due to Hopfield and Wolff cannot realistically explain the phase-angle dependence of the degree of polarization observed at small phase angles. The so-called interference or coherent backscattering mechanism is the most promising model. Models based on that mechanism use well-defined physical parameters to explain both negative polarization and the opposition effect. They are supported by laboratory experiments, particularly those showing enhancement of negative polarization with decreasing particle size down to the wavelength of light. According to the interference mechanism, pronounced negative branches of polarization, like those of C-class asteroids, may indicate a high degree of optical inhomogeneity of light-scattering surfaces at small scales. The mechanism also seems appropriate for treating the negative polarization and opposition effects of cometary dust comae, planetary rings, and the zodiacal light. 相似文献
9.
Hubert Halloin 《Experimental Astronomy》2005,20(1-3):171-184
Based on the laws of X-ray diffraction in crystals, Laue lenses offer a promising way to achieve the sensitivity and angular resolution leap required for the next generation of hard X-ray and gamma-ray telescopes.The present paper describes the instrumental responses of Laue diffraction lenses designed for nuclear astrophysics. Different possible geometries are discussed, as well as the corresponding spectral and imaging capabilities. These theoretical predictions are then compared with Monte-Carlo simulations and experimental results (ground and stratospheric observations from the CLAIRE project).
PACS 95.55.Ka, 61.50.Ah, 61.10.−i, 41.50.+h 相似文献
10.
Techniques to measure grain-size distributions of loamy sediments: a comparative study of ten instruments for wet analysis 总被引:2,自引:0,他引:2
DIRK GOOSSENS 《Sedimentology》2008,55(1):65-96
Ten instruments for measuring the grain‐size distribution of loamy sediments in water were tested in a comparative study. Instruments tested were: the Malvern Mastersizer S, the Coulter LS 200, the Fritsch Analysette 22 (version C), the Horiba Partica LA‐950, the Sedigraph 5100, the Atterberg cylinder, the Coulter Multisizer 3, the CIS‐100, the EyeTech and the image analysis software Histolab. The first four instruments use laser diffraction. The Sedigraph and Atterberg cylinder are based on sedimentation. The Coulter Multisizer 3 uses impedance measurements and the last three instruments use optical techniques. Grain‐size analyses were carried out on four sediments with median grain diameters of approximately 35, 30, 12 and 9 μm, respectively, and with no particles >90 μm. The laser diffraction instruments produced the best results for the various criteria considered in this study, followed by the Coulter Multisizer 3 (electrical sensing zone technique), the sedimentation techniques and the optical methods. However, the study also showed that there is no such thing as an ‘ideal’ method because techniques may score differently according to the criterion tested. An appropriate evaluation thus requires that various criteria be considered. Issues to be taken into account are: type of sediment, quantity of sediment available, speed of measurement, complexity of the measurement protocol, processing of the data, reproducibility of the results and the specific aims of the study undertaken. 相似文献