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91.
E. Tavarnelli 《International Journal of Earth Sciences》1996,85(2):363-371
The Umbria-Marche foreland fold-and-thrust belt in the northern Apennines of Italy provides excellent evidence to test the
hypothesis of synsedimentary-structural control on thrust ramp development. This orogenic belt consists of platform and pelagic
carbonates, Late Triassic to Miocene in age, whose deposition was controlled by significant synsedimentary extension. Normal
faulting, mainly active from Jurassic through Late Cretaceous-Paleogene time, resulted in significant lateral thickness variability
within the related stratigraphic sequences. By Late Miocene time the sedimentary cover was detached from the underlying basement
and was deformed by east-verging folds and west-dipping thrusts. Two restored balanced cross sections through the southernmost
part of the belt show a coincidence between the early synsedimentary normal faults and the late thrust fault ramps. These
evidences suggest that synsedimentary tectonic structures, such as faults and the related lithological lateral changes, can
be regarded as mechanically important controlling factors in the process of thrust ramp development during positive tectonic
inversion processes. 相似文献
92.
Kusuma G. Rao V. N. Lykossov A. Prabhu S. Sridhar E. Tonkacheyev 《Journal of Earth System Science》1996,105(3):227-260
An attempt has been made here to study the sensitivity of the mean and the turbulence structure of the monsoon trough boundary
layer to the choice of the constants in the dissipation equation for two stations Delhi and Calcutta, using one-dimensional
atmospheric boundary layer model withe-ε turbulence closure. An analytical discussion of the problems associated with the constants of the dissipation equation is
presented. It is shown here that the choice of the constants in the dissipation equation is quite crucial and the turbulence
structure is very sensitive to these constants. The modification of the dissipation equation adopted by earlier studies, that
is, approximating the Tke generation (due to shear and buoyancy production) in theε-equation by max (shear production, shear + buoyancy production), can be avoided by a suitable choice of the constants suggested
here. The observed turbulence structure is better simulated with these constants. The turbulence structure simulation with
the constants recommended by Aupoixet al (1989) (which are interactive in time) for the monsoon region is shown to be qualitatively similar to the simulation obtained
with the constants suggested here, thus implying that no universal constants exist to regulate dissipation rate.
Simulations of the mean structure show little sensitivity to the type of the closure parameterization betweene-l ande-ε closures. However the turbulence structure simulation withe-ε. closure is far better compared to thee-l model simulations. The model simulations of temperature profiles compare quite well with the observations whenever the boundary
layer is well mixed (neutral) or unstable. However the models are not able to simulate the nocturnal boundary layer (stable)
temperature profiles. Moisture profiles are simulated reasonably better. With one-dimensional models, capturing observed wind
variations is not up to the mark. 相似文献
93.
M. R. Handy 《International Journal of Earth Sciences》1996,85(4):832-851
The Zone of Samedan is part of a fossil, early Mesozoic rift system originally situated in the distal, Lower Austro-Alpine
domain of the Adriatic passive continental margin. An early Mesozoic configuration of asymmetrical rift basins bounded by
relative structural highs compartmentalized Late Cretaceous active margin tectonics; Jurassic half-grabens were folded into
arcuate synclines, whereas relative structural highs engendered thin, imbricated thrust sheets. West-directed thrusting and
folding initiated at the surface and continued to depths favoring mylonitization under lower greenschist-facies conditions.
At this time Liguria-Piemontese ophiolites were accreted to Lower Austro-Alpine units directly underlying the Zone of Samedan.
Late Cretaceous orogenic collapse of the Adriatic active margin involved the reactivation of west-directed thrusts as low-angle,
top-to-the-east, normal faults. These faults accommodated extensional uplift of Liguria-Piemontese ophiolites and Lower Austro-Alpine
units beneath and within the Zone of Samedan. During Paleogene collision, some Late Cretaceous faults in the Zone of Samedan
were reactivated under lower anchizonal conditions as north-directed thrusts. The latter stages of this early Tertiary thickening
were transitional to brittle, high-angle normal faulting associated with top-to-the-east extension and spreading above the
warm, uplifting Lepontine dome. 相似文献
94.
本文针对加拿大地球物理学家EdoNgland教授提出的问题,对M—P广义逆矩阵的递推算法进行了探分论述探讨的初步结果和对Greville递推算法的扩充。文中对算法的扩充给出严格的证明。 相似文献
95.
模拟退火剩余静校正的一步算法 总被引:1,自引:1,他引:1
当地震资料的剩余静校正量大、信噪比低时,利用传统的线性反演方法不能有效地拾取静校正量。本文介绍一种非线性反演方法(一步模拟退火法)来估算炮点和检波点的剩余静校正量。通过对合成地震记录的试算表明,该算法可获得近似于真实的剩余静校正量。 相似文献
96.
层析成像中的波形反演 总被引:1,自引:0,他引:1
在波动方程有限差分数值模拟基础上,用波形记录残差平方并建立目标函数。对目标函数进行梯度优化,我们得出了介质速度的迭代公式。通过计算目标函数梯度我们可以对介质进行速度校正,从而获得反演解。经数值试验证明这是一种很有效的反演方法。 相似文献
97.
用快速准确重力三维正演算法计算白垩系顶面及以上各密度界面的重力异常,采用“剥皮法”从实测重力异常中减去自垩系顶面及以上各密度界面的重力效应后得到剩余异常,由此反演研究区内白垩系底面深度。由于采用快速三维反演算法并顾及地质及航磁异常信息,求得了白垩系厚度,计算出的底板埋深等更为合理、精细,为洞庭地区油气资源基础性研究及评价提供了重要的信息。 相似文献
98.
揭示一个基于代数拓扑理论的裂隙网络中物质弥散模型,还给出了应用于网络中的对流扩散的对应性原理的证明。应用拓扑理论给出的框架,使其起了一个数据结构的组织者的作用,由此得到网络中每一个分支上的浓度的解。这个解是在拉普拉斯空间上的解析解。网络中任意点在任何时刻的浓度可以很方便地用数值拉氏反变换求出。 相似文献
99.
井间电阻率层析成象是一种探测地下浅部精细结构的物探方法,它主要用于解决工程地质问题。本文采用2.5-D有限元法,针对井间电阻率层析成象中的AM观测系统进行了反演成象计算。文中首先计算了灵敏度矩阵,然后给出了一种电阻率层析成象反演算法—平滑度约束反演,理论模型的计算和实际资料的处理,都证明了该算法的有效性 相似文献
100.
本文从最大后验概率密度观点出发,在数据噪音向量和待求模型向量为具有零均值的独立高斯随机过程的假设前提下,建立起了随机反演的非线性系统方程;给出了模型方差估计的函数表达式,并在文章最后,证明了反演解的稀疏性,即解释了随机反演的输出解的高分辨率特征。文章在最小二乘反演方法的基础上,发展并完善了随机反演方法的理论基础;揭示了随机反演方法与最小二乘反演方法之间的本质区别;阐述了随机反演方法的优越性,并指出了其广阔的应用前景。 相似文献