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   257180篇
  免费   5229篇
  国内免费   3315篇
测绘学   6861篇
大气科学   19092篇
地球物理   53780篇
地质学   89317篇
海洋学   21498篇
天文学   56094篇
综合类   1018篇
自然地理   18064篇
  2021年   2189篇
  2020年   2597篇
  2019年   2860篇
  2018年   3495篇
  2017年   3246篇
  2016年   5694篇
  2015年   4212篇
  2014年   6898篇
  2013年   14201篇
  2012年   6470篇
  2011年   7824篇
  2010年   6913篇
  2009年   9496篇
  2008年   8351篇
  2007年   7851篇
  2006年   9664篇
  2005年   7705篇
  2004年   7619篇
  2003年   7129篇
  2002年   6680篇
  2001年   5963篇
  2000年   5939篇
  1999年   5200篇
  1998年   5224篇
  1997年   5021篇
  1996年   4655篇
  1995年   4407篇
  1994年   4096篇
  1993年   3829篇
  1992年   3604篇
  1991年   3580篇
  1990年   3747篇
  1989年   3501篇
  1988年   3302篇
  1987年   3845篇
  1986年   3401篇
  1985年   4218篇
  1984年   4726篇
  1983年   4407篇
  1982年   4314篇
  1981年   3914篇
  1980年   3642篇
  1979年   3513篇
  1978年   3483篇
  1977年   3281篇
  1976年   3042篇
  1975年   2964篇
  1974年   2920篇
  1973年   3079篇
  1972年   2026篇
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
851.
A nonlinear process for the resonant generation of low-frequency fast magnetosonic kink waves in coronal loops is discussed. The efficiency of the process is strongly enhanced due to the existence of a nonlinearly selected frequency produced by a constant frequency difference in the dispersion curves in the short wavelength limit. The kink wave with the selected frequency interacts with high-frequency kink and sausage waves. The efficiency of such interaction does not require coherence in the interactive waves. In a loop of width 2 × 103 km, field strength 50 G and number density 5 × 1015 m–3, the nonlinearly selected frequency is of order 46 mHz (period 21.8 s), but this may range through 11 mHz to 184 mHz (periods 86.5 s to 5.4 s) for typical coronal conditions.  相似文献   
852.
The spectra of active galaxies and their nuclei are rich in emission and absorption line features. A major aim of present research is the development of self-consistent hydrodynamic models for the production of the line-forming regions. We here review such modelling and stress the central role played by shock phenomena induced by winds and explosions on scales ranging from the circumstellar to the intergalactic.  相似文献   
853.
854.
New aeromagnetic data, K-Ar age determinations of dredged marine igneous rocks, as well as other geophysical evidence have shed light on the chronology, nature and evolution of the northern Iceland Plateau. Correspondence between seismic refraction profiles taken on the Jan Mayen Ridge and westward through Jan Mayen Island, suppressed aeromagnetic anomalies, earthquake surface wave studies, and ages of dredged igneous rocks suggest these strata may form an extended region of thickened crust, possibly of Caledonian age, extending westward toward the Kolbeinsey Ridge and northwest to the south wall of the Jan Mayen Fracture Zone.  相似文献   
855.
The oscillatory, conjugate and asymptotic behaviours of the principal and non-principal solutions of the Blasius and corresponding heat transfer equations governing the compressible laminar boundary-layer flow over a semi-infinite flat plate with heat flux have been studied; the results of the discussion being based on the asymptotic integrations of second-order linear differential equations.  相似文献   
856.
The Indian team at ISRO has been part of the Whole Earth Telescope (WET) team since 1988 when we first participated in the campaign on V471 Tau. We have been part of many other observing campaigns over the last decade. This presentation traces the circumstances leading to our joining the WET team and how useful the coverage from the Indian longitude has been. The results of several pulsators from the WET runs during which we participated are also described. These include PG1159-035 the prototype of the GW Vir type of stars, RE J 0751+14 a cataclysmic variable, PG 1336-018 a binary with an sdB pulsator and finally HR 1217 a roAp star. The paper concludes with what the limitations are in our observations and how we can overcome them in the future.  相似文献   
857.
858.
859.
860.
In experiments at the high-power Z-facility at Sandia National Laboratory in Albuquerque, New Mexico, we have been able to produce a low density photoionized laboratory plasma of Fe mixed with NaF. The conditions in the experiment allow a meaningful comparison with X-ray emission from astrophysical sources. The charge state distributions of Fe, Na and F are determined in this plasma using high resolution X-ray spectroscopy. Independent measurements of the density and radiation flux indicate unprecedented values for the ionization parameter ξ = 20–25 erg cm s−1 under nearly steady-state conditions. First comparisons of the measured charge state distributions with X-ray photoionization models show reasonable agreement, although many questions remain.  相似文献   
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