首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   71714篇
  免费   853篇
  国内免费   619篇
测绘学   1944篇
大气科学   5125篇
地球物理   12917篇
地质学   28049篇
海洋学   6036篇
天文学   15727篇
综合类   308篇
自然地理   3080篇
  2022年   365篇
  2021年   622篇
  2020年   659篇
  2019年   708篇
  2018年   3943篇
  2017年   3649篇
  2016年   3107篇
  2015年   1076篇
  2014年   1774篇
  2013年   2868篇
  2012年   2718篇
  2011年   4609篇
  2010年   4083篇
  2009年   4774篇
  2008年   3939篇
  2007年   4577篇
  2006年   2227篇
  2005年   2012篇
  2004年   1941篇
  2003年   1901篇
  2002年   1698篇
  2001年   1324篇
  2000年   1249篇
  1999年   994篇
  1998年   1038篇
  1997年   947篇
  1996年   815篇
  1995年   781篇
  1994年   684篇
  1993年   602篇
  1992年   590篇
  1991年   593篇
  1990年   622篇
  1989年   493篇
  1988年   503篇
  1987年   528篇
  1986年   487篇
  1985年   610篇
  1984年   673篇
  1983年   590篇
  1982年   561篇
  1981年   511篇
  1980年   487篇
  1979年   477篇
  1978年   458篇
  1977年   368篇
  1976年   349篇
  1975年   357篇
  1974年   308篇
  1973年   342篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
211.
We examine time variations of the total magnetospheric output UT and the two geomagnetic indices AE and Dst during the magnetospheric storm of 31 December 1967–1 January 1968. A unique feature of this particular storm is that the solar-wind magnetosphere dynamo power ε was nearly constant for about 24 h by maintaining a high value of ~1019 erg s?1. It is found that UT was also nearly constant during that period, indicating that the magnetosphere is primarily a directly driven system. However, during an early epoch of the storm, the electrojet intensity levelled off, while the ring current began to grow during the same epoch. Subsequently, there occurred a sudden surge of the electrojet intensity, while the growth of the ring-current levelled off. Later variations of both the AE and Dst indices were very complex. After the surge, the AE index continued to decline and became as low as ~250 nT during the maximum epoch of this major storm (when the Dst decrease attained the maximum values). This trend can also be seen in many other major storms, but is often masked by changes of ε. One possible cause for such features for ε ? 1019erg/s?1 is that the neutral wind is generated by the (E × B) motion in the lower ionosphere, reducing the electrojet intensity and enhancing the ring-current particle-injection rate.  相似文献   
212.
The accuracy of the AE index as a measure of the joule heat production rate is examined for a typical substorm event on 18 March 1978 by estimating the global joule heat production rate, as a function of time, using data obtained from the IMS six meridian chains. In spite of the fact that the AE index had had an initial slow growth which was followed by a rapid growth, the joule heat production rate attained a high level during the slow growth and thus their variations were considerably different from those of the AE index. Therefore, although the AE index is statistically linearly related to the global joule heat production rate, one should be cautious in assuming that details of time variations of the AE index during individual events represent those of the joule heat production rate.  相似文献   
213.
We investigate the evolution of rotation period and spindown age of a pulsar whose surface magnetic field undergoes a phase of growth. Application of these results to the Crab pulsar strongly indicates that its parameters cannot be accounted for by the field growth theories.  相似文献   
214.
The treatment followed by Coxet al. (1973) for the estimation of the effects of thermal imbalance on the pulsational stability of stars is applied to Roche and point source (Chandrika Prashad) model. The calculations suggest that the eigenvalues obtained for the above model are correct to 0(t ff/ts). The expressions for stability coefficients and corresponding eigenfunctions for the stars in thermal imbalance for the above models have also been derived.  相似文献   
215.
The crab Carcinus maenas (L.) and the barnacle Elminius modestus Darwin were exposed to a range of dissolved concentrations of Zn, Cu and Cd for 21 days in artificial seawater. Accumulation of Zn and Cu by crabs has been interpreted in terms of the presence of a regulation mechanism to maintain constant body concentrations (83·2 ± 19·4 μg Zn g?1 dry wt.; 39·8 ± 9·8 μg Cu g?1 dry wt.) under varying external dissolved metal levels, until a threshold dissolved metal concentration (c. 400 μg Zn l?1; c. 170 μg Cu l?1) beyond which net accumulation of metal begins. Cadium appears to be accumulated by C. maenas at all exposures with no evidence for regulation of body cadmium concentrations. Exposure of E. modestus to Zn, Cu or Cd caused net accumulation of the respective metal in the bodies of the barnacles, with no evidence for regulation of body metal concentrations.  相似文献   
216.
The proposed baseline GAIA mission will be able to detect the astrometric signature of Jupiter-size planets around of the order of a million stars, using either global or narrow-angle astrometry. If the mission can realize the higher astrometric accuracy that photon statistics allows for bright stars, lower-mass planets (from Earth size to ten times larger) can be found around ten to a few hundred stars.  相似文献   
217.
The main analytical properties of the generalized Shkarofsky function and a numerical code for its computation are discussed. The results of a numerical analysis are compared with the results of an asymptotic analysis for parameter values relevant to the problem of whistler-mode propagation in the Earth's magnetosphere. This comparison allows us to specify the range of applicability of different approximations to the generalized Shkarofsky function, which have been used for the analysis of relativistic effects on whistler-mode propagation and instability.  相似文献   
218.
219.
Observations and recommendations of the second un/esa workshop on basic space science  相似文献   
220.
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号