全文获取类型
收费全文 | 83765篇 |
免费 | 1333篇 |
国内免费 | 1419篇 |
专业分类
测绘学 | 2534篇 |
大气科学 | 6363篇 |
地球物理 | 16111篇 |
地质学 | 32739篇 |
海洋学 | 6720篇 |
天文学 | 17394篇 |
综合类 | 483篇 |
自然地理 | 4173篇 |
出版年
2022年 | 438篇 |
2021年 | 717篇 |
2020年 | 691篇 |
2019年 | 771篇 |
2018年 | 4080篇 |
2017年 | 3829篇 |
2016年 | 3243篇 |
2015年 | 1343篇 |
2014年 | 1914篇 |
2013年 | 3368篇 |
2012年 | 3090篇 |
2011年 | 5077篇 |
2010年 | 4538篇 |
2009年 | 5243篇 |
2008年 | 4342篇 |
2007年 | 4921篇 |
2006年 | 2714篇 |
2005年 | 2448篇 |
2004年 | 2171篇 |
2003年 | 2145篇 |
2002年 | 1935篇 |
2001年 | 1525篇 |
2000年 | 1497篇 |
1999年 | 1252篇 |
1998年 | 1247篇 |
1997年 | 1221篇 |
1996年 | 1069篇 |
1995年 | 1031篇 |
1994年 | 902篇 |
1993年 | 816篇 |
1992年 | 765篇 |
1991年 | 758篇 |
1990年 | 811篇 |
1989年 | 732篇 |
1988年 | 671篇 |
1987年 | 821篇 |
1986年 | 678篇 |
1985年 | 824篇 |
1984年 | 962篇 |
1983年 | 864篇 |
1982年 | 846篇 |
1981年 | 743篇 |
1980年 | 762篇 |
1979年 | 648篇 |
1978年 | 620篇 |
1977年 | 604篇 |
1976年 | 545篇 |
1975年 | 528篇 |
1974年 | 562篇 |
1973年 | 623篇 |
排序方式: 共有10000条查询结果,搜索用时 9 毫秒
101.
OSCR is an HF radar system that has been developed for high spatial resolution coastal surface current measurement. This paper describes preliminary results that demonstrate that wave measurement can be successfully obtained from suitably processed OSCR data. Comparisons with data from a WAVEC directional buoy are presented and show encouraging agreement. Some of the limitations to the measurement process are discussed and indicate a maximum range of about 20 km. Surface current variability on short time scales presents the most serious obstacle to wave measurement. This appears to be more of a problem when the mean currents are large, in that in these circumstances the data fail initial quality control criteria. However, in lower mean currents, the effect is often still present and leads to errors in long wave measurement 相似文献
102.
Infiltration experiments have been performed at three sites along a well-known catena under virgin tropical rain forest using a portable sprinkling infiltrometer. Experimentally determined infiltration curves are presented. Infiltration curves are also simulated on the basis of the Mein-Larson equation. The parameters for this model have been obtained from the infiltration curves (saturated conductivity) and simple soil moisture determinations (fillable porosity). The agreement between experimentally determined and modelled infiltration is reasonable, provided (a) saturated conductivity as derived from the experimental data is corrected, (b) a storage parameter, also derived from the experimental data, is added to the Mein-Larson model, and (c) the decline in soil porosity with depth is either small or occurs abruptly at shallow depth. Comparison of observed infiltration rates with rainfall intensity shows that Horton Overland Flow has to occur naturally at least on the middle and lower section of the catena. Despite the fact that most parameters can be estimated in principle from basic soil data, it remains advisable to obtain sprinkling infiltrometer field measurements, because of soil variability due to dynamic surface conditions, macroporosity, air entrapment, and irregularity of the wetting front. 相似文献
103.
104.
In this paper we consider the time-dependent diffuse reflection and transmission problems for a homogeneous anisotropically-scattering atmosphere of finite optical depth and solve it by the principle of invariance. Also we consider the time-dependent diffuse reflection and transmission of parallel rays by a slab consisting of two anisotropic homogeneous layers, whose scattering and transmission properties are known. It is shown how to express the time-dependent reflected and transmitted intensities in terms of their components. In a manner similar to that given by Tsujita (1968), we assumed that the upward-directed intensities of radiation at the boundary of the two layers are expressed by the sum of products of some auxiliary functions depending on only one argument. Then, after some analytical manipulations, three groups of systems of simultaneous integral equations governing the auxiliary functions are obtained. 相似文献
105.
106.
B. R. Johnson M. E. Abroe P. Ade J. Bock J. Borrill J. S. Collins P. Ferreira S. Hanany A. H. Jaffe T. Jones A. T. Lee L. Levinson T. Matsumura B. Rabii T. Renbarger P. L. Richards G. F. Smoot R. Stompor H. T. Tran C. D. Winant 《New Astronomy Reviews》2003,47(11-12):1067
We discuss MAXIPOL, a bolometric balloon-borne experiment designed to measure the E-mode polarization anisotropy of the cosmic microwave background radiation (CMB) on angular scales of 10′ to 2°. MAXIPOL is the first CMB experiment to collect data with a polarimeter that utilizes a rotating half-wave plate and fixed wire-grid polarizer. We present the instrument design, elaborate on the polarimeter strategy and show the instrument performance during flight with some time domain data. Our primary dataset was collected during a 26 h turnaround flight that was launched from the National Scientific Ballooning Facility in Ft. Sumner, New Mexico in May 2003. During this flight five regions of the sky were mapped. Data analysis is in progress. 相似文献
107.
108.
109.
The effect of particle-particle interaction on the adiabatic index γ for an electron-positron plasma is considered. An improved method for numerically calculating the Hartree-Fock exchange integral is presented and its relativistic asymptotics is determined. An approximation formula is derived for the correlation part of the interaction in the low-density limit. This formula includes degeneracy and the positron component. 相似文献
110.
A high-velocity ionized outflow and XUV photosphere in the narrow emission line quasar PG1211+143 总被引:1,自引:0,他引:1
K. A. Pounds J. N. Reeves A. R. King K. L. Page P. T. O'Brien M. J. L. Turner 《Monthly notices of the Royal Astronomical Society》2003,345(3):705-713
We report on the analysis of a ∼60-ks XMM–Newton observation of the bright, narrow emission line quasar PG1211+143. Absorption lines are seen in both European Photon Imaging Camera and Reflection Grating Spectrometer spectra corresponding to H- and He-like ions of Fe, S, Mg, Ne, O, N and C. The observed line energies indicate an ionized outflow velocity of ∼24 000 km s−1 . The highest energy lines require a column density of N H ∼ 5 × 1023 cm−2 , at an ionization parameter of log ξ∼ 3.4 . If the origin of this high-velocity outflow lies in matter being driven from the inner disc, then the flow is likely to be optically thick within a radius of ∼130 Schwarzschild radii, providing a natural explanation for the big blue bump (and strong soft X-ray) emission in PG1211+143. 相似文献