全文获取类型
收费全文 | 66169篇 |
免费 | 1121篇 |
国内免费 | 493篇 |
专业分类
测绘学 | 1634篇 |
大气科学 | 5272篇 |
地球物理 | 13730篇 |
地质学 | 21402篇 |
海洋学 | 5715篇 |
天文学 | 15214篇 |
综合类 | 133篇 |
自然地理 | 4683篇 |
出版年
2020年 | 473篇 |
2019年 | 495篇 |
2018年 | 933篇 |
2017年 | 916篇 |
2016年 | 1362篇 |
2015年 | 1011篇 |
2014年 | 1413篇 |
2013年 | 3235篇 |
2012年 | 1488篇 |
2011年 | 2271篇 |
2010年 | 1938篇 |
2009年 | 2918篇 |
2008年 | 2658篇 |
2007年 | 2390篇 |
2006年 | 2456篇 |
2005年 | 2132篇 |
2004年 | 2234篇 |
2003年 | 2060篇 |
2002年 | 1963篇 |
2001年 | 1774篇 |
2000年 | 1746篇 |
1999年 | 1504篇 |
1998年 | 1490篇 |
1997年 | 1480篇 |
1996年 | 1272篇 |
1995年 | 1208篇 |
1994年 | 1090篇 |
1993年 | 994篇 |
1992年 | 943篇 |
1991年 | 799篇 |
1990年 | 1008篇 |
1989年 | 848篇 |
1988年 | 753篇 |
1987年 | 927篇 |
1986年 | 817篇 |
1985年 | 1019篇 |
1984年 | 1181篇 |
1983年 | 1123篇 |
1982年 | 1016篇 |
1981年 | 976篇 |
1980年 | 833篇 |
1979年 | 815篇 |
1978年 | 867篇 |
1977年 | 787篇 |
1976年 | 749篇 |
1975年 | 696篇 |
1974年 | 703篇 |
1973年 | 708篇 |
1972年 | 440篇 |
1971年 | 384篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
181.
182.
183.
A one-dimensional model for thinning of the plasma sheet is developed on the basis of launching a fast mode MHD rarefaction wave propagating in the tailward direction along the plasma sheet. Behind the rarefaction wave the pressure is reduced, leading to thinning of the plasma sheet and also to an Earthward plasma flow with a speed on the order of the sound speed a0. The plasma sheet thickness is reduced by a factor of 2 if an Earthward plasma flow speed of 0.8a0 is induced. The predictions of the model are in reasonable agreement with observations. 相似文献
184.
A non-steady, two-dimensional, compressible mathematical model of a fluid with constant viscosity and thermal conductivity is given in order to represent a thin atmospheric layer located at 60 km height, as a function of a known initial vertical distribution of temperature, chemical concentrations of minor components and assumed free boundary conditions.The purpose of this paper is to determine the influence of convective laminar processes in the vertical distribution of minor constituents in a thermal interface. Only three minor components are considered, atomic oxygen, molecular oxygen and ozone. Numerical solutions of the stated timedependent convection problem for different Rayleigh numbers show a marked influence of the established flow pattern upon the distribution of minor constituents. In all cases, an enhancement of mean concentration gradients in relatively small regions adjacent to the warmer and colder boundaries was observed. 相似文献
185.
D.J. Southwood 《Planetary and Space Science》1977,25(6):549-554
It is shown that the field line resonance phenomenon that occurs for quasi-transverse signals in a non-uniform cold plasma generally occurs for disturbances with a compressional magnetic component in a hot plasma like the ring current. The equations describing such localised signals are derived and discussed in various limits. It is pointed out that recent observations of low frequency compressional oscillations on spacecraft may be an example of such localised signals. 相似文献
186.
Intensive partial reflection drift observations were made at Adelaide (35°S) for a seven day period in June 1973. The results have been analysed to isolate the prevailing motion and oscillations of various time scales: planetary, 24 hr, 12 hr and gravity waves. Each is discussed in turn with particular emphasis on the variability of energy from day to day and as a function of height. Evidence is presented for the local generation of planetary waves, the presence of the evanescent S?21 mode in the 24 hr oscillation, the influence of the S42 mode in the 12 hr oscillation and a definite polarization of gravity waves. The energies of all the forms of motion are shown to decay exponentially with increasing height and the deposition of energy and momentum in the upper mesosphere and lower thermosphere is discussed. 相似文献
187.
188.
Some properties of the recently-discovered torsional oscillations of the Sun are presented. The detailed relation of this velocity feature to magnetic activity gives evidence that these motions represent a fundamental oscillation within the Sun that is responsible for the solar activity cycle and that they are not a natural consequence of an - dynamo. A new torsional oscillation with wave number 1 hemisphere–1 is demonstrated to exist on the Sun. 相似文献
189.
A numerical test is made to determine if the high-latitude torsional wave is generated from the low-latitude torsional pattern as a result of our reduction procedures. The results indicate that the high-latitude motions are not an artifact of the analysis, but are true solar features. We demonstrate also that the one-wave-per-hemisphere torsional oscillation does not result from the reduction procedure. These results place the observations in conflict with the predictions of - () models of the solar cycle.Now at Institute for Astronomy, University of Hawaii, Honolulu, Hawaii 96822, U.S.A. 相似文献
190.
The authors attempt to provide a comprehensive review of urbanization in three Melanesian countries (Papua New Guinea, the Solomon Islands, and Vanuatu) and in Fiji. The focus of the paper is on the development and perpetuation of various forms of inequality exemplified by Melanesian urbanization and its colonial origins. 相似文献