全文获取类型
收费全文 | 15879篇 |
免费 | 3533篇 |
国内免费 | 4960篇 |
专业分类
测绘学 | 2268篇 |
大气科学 | 2931篇 |
地球物理 | 3046篇 |
地质学 | 9083篇 |
海洋学 | 2785篇 |
天文学 | 463篇 |
综合类 | 1389篇 |
自然地理 | 2407篇 |
出版年
2024年 | 102篇 |
2023年 | 338篇 |
2022年 | 900篇 |
2021年 | 1007篇 |
2020年 | 914篇 |
2019年 | 979篇 |
2018年 | 954篇 |
2017年 | 878篇 |
2016年 | 902篇 |
2015年 | 997篇 |
2014年 | 1030篇 |
2013年 | 1208篇 |
2012年 | 1289篇 |
2011年 | 1332篇 |
2010年 | 1215篇 |
2009年 | 1180篇 |
2008年 | 1159篇 |
2007年 | 1111篇 |
2006年 | 1051篇 |
2005年 | 849篇 |
2004年 | 690篇 |
2003年 | 474篇 |
2002年 | 522篇 |
2001年 | 477篇 |
2000年 | 446篇 |
1999年 | 351篇 |
1998年 | 253篇 |
1997年 | 238篇 |
1996年 | 217篇 |
1995年 | 190篇 |
1994年 | 180篇 |
1993年 | 151篇 |
1992年 | 148篇 |
1991年 | 124篇 |
1990年 | 94篇 |
1989年 | 79篇 |
1988年 | 64篇 |
1987年 | 57篇 |
1986年 | 37篇 |
1985年 | 27篇 |
1984年 | 24篇 |
1983年 | 17篇 |
1982年 | 30篇 |
1981年 | 15篇 |
1980年 | 8篇 |
1979年 | 14篇 |
1977年 | 6篇 |
1976年 | 8篇 |
1957年 | 6篇 |
1954年 | 4篇 |
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
31.
Numerical methods are usually used for the computation of ephemerides with perturbations for the precise orbital determination of an artificial satellite. But their numerical stability will be encountered in a long arc. In this case the use the improved Encke special perturbation methods has been suggested. The results of this paper show that Encke's method does indeed have a certain effectiveness, but cannot yet completely resolve the numerical stability, and the more efficient method is to use the energy integral or its variational relation to control the growth of the along-track error in general numerical calculations so that the aim of stabilization can be achieved. 相似文献
32.
33.
Hong Lin Zhang Douglas H. Sampson 《Monthly notices of the Royal Astronomical Society》2001,322(3):433-437
Calculations are made of the resonance contribution to electron-impact excitation of H-like 13 C and Li-like 23 Na, 25 Mg, 27 Al and 29 Si to the upper hyperfine levels that produce millimetre (mm) lines of likely astrophysical interest. The resonance contribution is found to be very important for these Li-like ions, considerably more important than for Li-like 57 Fe considered previously. However, resonances are found to be rather unimportant for H-like 13 C. The effect of radiative decay on the resonance contribution is found to be insignificant in all of the present calculations. 相似文献
34.
35.
活动星系核(AGN)是宇宙中最奇特的天体之一。它是真正意义上的全波天体,其中X射线波段的发射功率占到全波段功率的50%左右。AGN的X射线辐射研究涉及天体物理中的最基本问题,例如能量产生、辐射机制和宇宙论等,而Chandra X射线卫星的高分辨率图像和光谱对这一研究有着重要作用。以Chandra卫星的部分观测结果为例,简要介绍了几类不同类型AGN的X射线辐射研究进展:(1)宽吸收线类星体APM08279+5255(z=3.91)的X射线谱分析,以及高红移类星体的观测概况;(2)Seyfert星系NGC 4151延展X射线发射问题的解决,及NGC 1068X射线辐射与光学波段的高激发态发射线([OⅢ]λ5007)有很强相关性的发现;(3)6个BLLac天体样本的X射线环境分析;(4)射电星系X射线喷流的观测等。 相似文献
36.
在社会发展的层面上认识“数字地球” 总被引:1,自引:0,他引:1
本文讨论了“数字地球”的有关问题。指出“数字地球”是人类社会及其活动在网络空间的延伸和拓展,是信息技术带来的社会发展趋势。关于“数字地球”的讨论不应局限在空间信息技术领域,而应该在社会发展的层面上认识它 相似文献
37.
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
38.
The paper presents a simple approximate analytical solution of the remote stresses that cause the collapse of a borehole or other circular cylindrical cavity in an infinite elastic space. Regions of parallel equidistant splitting cracks are assumed to form on the sides of the cavity. Their boundary is assumed to be an ellipse of a growing horizontal axis, the other axis remaining equal to the borehole diameter. The slabs of rock between the splitting cracks are assumed to buckle as slender columns, and their post-critical stress is considered as the residual stress in the cracked rock. The buckling of these slab columns is assumed to be resisted not only by their elastic bending stiffness but also shear stresses produced on rough crack faces by relative shear displacements. The energy release from the infinite medium caused by the growth of the elliptical cracking region is evaluated according to Eschelby's theorem. This release is set equal to the energy dissipated by the formation of all the splitting cracks, which is calculated under the assumption of constant fracture energy. This yields the collapse stress as a function of the elastic moduli, fracture energy, ratio of the remote principal stresses, crack shear resistance characteristic and borehole diameter. The collapse stress as a function of crack spacing is found to have a minimum, and the correct crack spacing is determined from this minimum. For small enough diameters, the crack spacing increases as the (4/5)-power of the borehole diameter, while for large enough diameters a constant spacing is approached. In contrast to plastic solutions, the breakout stress exhibits a size effect, such that for small enough diameters the breakout stress decreases as the (? 2/5)-power of the borehole diameter, while for large enough diameters a constant limiting value is approached. Finally, some numerical estimates are given and the validity of various simplifying assumptions made is discussed. 相似文献
39.
地倾斜台站数字化、模拟观测数据频率特性研究 总被引:2,自引:2,他引:0
分析了四川、云南的部分地倾斜数字化观测与模拟观测资料的特性,从频率范围,周期10天以上的FFT谱特性,固体潮波振幅,相位特征值等方面,论述了地倾斜数字化资料较模拟记录资料的信息组成变化,并对资料的分析与应用进行了初步探讨。 相似文献
40.
Silvio Lorenzetti Yangting Lin Daode Wang Otto Eugster 《Meteoritics & planetary science》2003,38(8):1243-1253
Abstract— We determined the mineralogical and chemical characteristics and the He, Ne, and Ar isotopic abundances of 2 meteorites that fell in China and of 2 meteorites that were recovered by the 15th Chinese Antarctic Research Expedition. Guangmingshan (H5), Zhuanghe (H5), and Grove Mountain (GRV) 98002 (L5) yield cosmic ray exposure (CRE) ages of 68.7 ± 10.0 Ma, 3.8 ± 0.6 Ma, and 17.0 ± 2.5 Ma, respectively. These ages are within the range typically observed for the respective meteorite types. GRV 98004 (H5) had an extremely short parent body‐Earth transfer time of 0.052 ± 0.008 Ma. Its petrography and mineral chemistry are indistinguishable from other typical H5 chondrites. Only 3 other meteorites exist with similarly low CRE ages: Farmington (L5), Galim (LL6), and ALH 82100 (CM2). We show that several asteroids in Earth‐crossing orbits, or in the main asteroid belt with orbits close to an ejection resonance, are spectrally matching candidates and may represent immediate precursor bodies of meteorites with CRE ages ≤0.1 Ma. 相似文献