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731.
X射线荧光光谱法直接测定地质样品中多种痕量元素 总被引:2,自引:0,他引:2
采用低压聚乙烯镶边垫底的粉末压饼法制样,X射线荧光光谱法直接测定了地质样品中痕量元素As、Ga、Sc、La、Y、Ce、W、Mo、Sn、Co和Pb。讨论了背景校正、谱线重叠校正、基体效应校正和仪器漂移校正等问题。利用理论α系数代替经验系数,使方法具有较高的准确度和较低的检出限。所测11个元素的检出限在(0.30~2.02)×10-6水平,精度(RSD,n=11)在0.95%~13.0%。方法经国家一级标准物质分析验证,结果与标准值相符。 相似文献
732.
对混合相中硅线石和莫来石的X射线衍射定性,定量分析表明,选取硅线石的d(332)S峰,莫来石的d(331)M峰或硅线石的d(220)S峰,莫来石的d(220)M峰放慢扫描速度,可定性分析硅线石和莫来石;选取硅线石的d(332)S峰,莫来石的d(331)M峰,采用计算机拟合分峰改进自清洗法,可定量分析硅线石和莫来石。经电子探针验证,实验方法准确,可行。 相似文献
733.
A. Akhperjanian R. Kankanian V. Sahakian A. Heusler C.-A. Wiedner H. Wirth 《Experimental Astronomy》1998,8(2):135-152
The raytracing technique was used to derive a suitable design for the HEGRA system of Cherenkov telescopes, which is at present commissioned at La Palma. The reflectors with a diameter of 3.9 m consist of 30 spherical mirrors with focal lengths in the range of 4.88 – 4.94 m. It is shown that 93% of the photons from the Cherenkov light emitted by an extended air shower are contained in the camera pixels, 0.25° in diameter, for the full field of view of = ± 2.5°. The optical performance of the HEGRA design is compared to other layouts. 相似文献
734.
Pseudo-bending method for three-dimensional seismic ray tracing in a spherical earth with discontinuities 总被引:7,自引:0,他引:7
We present a 'pseudo-bending' approach to 3-D ray tracing in a spherical earth with discontinuities. This method is based on a three-point perturbation associated with a first-order approximation, while Snell's law in curvilinear coordinates is applied at the discontinuities. We demonstrate the computational accuracy and efficiency of the pseudo-bending method in tracing rays for various velocity models by comparing results with analytical solutions and with results from the bending method. The improvement of efficiency is significant, but is reduced as the number of discontinuities increases. Since the bending approach may be computationally unstable in some situations, even though it is exact, the pseudo-bending approach is preferable for automatic calculation of rays. 相似文献
735.
介绍了纵波在地球内部的传播过程和浅源极远震的震相特点。由不同震中距的地震反映在三分向地震记录图上的初至震相振幅比的差异,归纳出由地震初动判别地震类型的方法,结合实际工作经验,得出如何判别PKS震相、如何由PP推S、由SS反推PP震相,以及根据地震面波的到时,通过《Rm-P》表来验证震中距等几种识别极远震及其震相的方法。 相似文献
736.
Statistics of traveltimes and amplitudes in random media 总被引:1,自引:0,他引:1
737.
738.
Ivo Opršal Johana Brokešová Donat Fäh Domenico Giardini 《Studia Geophysica et Geodaetica》2002,46(4):711-730
Hybrid approaches find broad applications wherever all-in-one modelling of source, path, and site effects is too expensive. Our new 3D hybrid approach allows to compute the seismic wavefield in elastic isotropic models containing a complex local structure embedded in a large, but considerably simpler, regional structure. The hybrid modelling is realized in two successive steps.In the 1st step, the ray or discrete wave number (DWN) method is used to compute the seismic wavefield due to the source and simple regional structure. The complex local structure is not present. Thus, the excitation contains the source and regional path effects. The time history of this wavefield (excitation), recorded at the points of so called excitation box, is stored on a disk. The excitation box envelopes a small portion of a computational domain.The 2nd step of the hybrid method, now containing the complex local structure, is computed by finite differences (FD) inside the excitation box and its close vicinity. The excitation from the 1st step is now used to inject the 1st step wavefield into the 2nd step computation. After that, the hybrid combination of the 1st and 2nd steps contains the source, regional path, and local structure effects at reasonably lower computational costs than in case of all-in-one modelling.The 3D ray-FD method is tested on models in which the locally complex structure is the well-known Volvi lake basin, embedded in various 1D structures. The wavefield is excited by the point source situated outside the basin. Although the structure outside the excitation box may be less dimensional (2D, 1D, homogeneous), the whole problem is actually 3D due to the 3D features of the structure inside the excitation box, 3D shape of the excitation box, and arbitrary source — excitation-box configuration. Simple (1D) structures outside the excitation box allow for comparison with the alternative hybrid DWN-FD results. However the ray method is suitable for computation of 3D regional structures outside the excitation box. The results from both approaches show a very good agreement for realistic crustal and local structural models. 相似文献
739.
P. Armstrong P. M. Chadwick P. J. Cottle J. E. Dickinson M. R. Dickinson N. A. Dipper S. E. Hilton W. Hogg J. Holder T. R. Kendall T. J. L. McComb C. M. Moore K. J. Orford S. M. Rayner I. D. Roberts M. D. Roberts M. Robertshaw S. E. Shaw K. Tindale S. P. Tummey K. E. Turver 《Experimental Astronomy》1999,9(2):51-80
740.
D. J. Buckley M. C. Dorrington P. J. Edwards T. J. L. McComb S. P. Tummey K. E. Turver 《Experimental Astronomy》1999,9(4):237-249
A technique for detecting the presence of cloud in the field of view of an atmospheric erenkov telescope using a mid infra red radiometer is described. Models for the radiative emission from clear and cloudy skies are tested and found to represent the measurements. 相似文献