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   106249篇
  免费   1655篇
  国内免费   1586篇
测绘学   3295篇
大气科学   7693篇
地球物理   20684篇
地质学   41273篇
海洋学   8269篇
天文学   20299篇
综合类   2351篇
自然地理   5626篇
  2022年   400篇
  2021年   723篇
  2020年   808篇
  2019年   871篇
  2018年   7607篇
  2017年   6856篇
  2016年   5383篇
  2015年   1628篇
  2014年   2312篇
  2013年   3897篇
  2012年   3778篇
  2011年   7055篇
  2010年   5968篇
  2009年   7067篇
  2008年   6067篇
  2007年   6711篇
  2006年   3017篇
  2005年   2928篇
  2004年   2909篇
  2003年   2791篇
  2002年   2324篇
  2001年   1883篇
  2000年   1822篇
  1999年   1411篇
  1998年   1516篇
  1997年   1397篇
  1996年   1119篇
  1995年   1153篇
  1994年   973篇
  1993年   880篇
  1992年   866篇
  1991年   772篇
  1990年   864篇
  1989年   730篇
  1988年   658篇
  1987年   820篇
  1986年   666篇
  1985年   866篇
  1984年   934篇
  1983年   874篇
  1982年   842篇
  1981年   735篇
  1980年   686篇
  1979年   613篇
  1978年   612篇
  1977年   558篇
  1976年   545篇
  1975年   499篇
  1974年   510篇
  1973年   471篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
451.
The southwest monsoon that dominated Central Himalaya has preserved loessic silt deposits preserved in patches that are proximal to periglacial areas. The occurrence of such silts suggests contemporary prevalence of cold and dry northwesterly winds. Field stratigraphy, geochemistry, mineral magnetism, infrared stimulated luminescence (IRSL) and radiocarbon dating has enabled reconstruction of an event chronology during the past 20 ka. Three events of loess accretion could be identified. The first two events of loess deposition occurred betweem 20 and 9 ka and were separated by a phase of moderate weathering. Pedogenesis at the end of this event gave rise to a well‐developed soil that was bracketed around 9 to > 4 ka. This was followed by the third phase of loess accretion that occurred around 4 to > 1 ka. Episodes of loess deposition and soil formation are interpreted in terms of changes in the strength of the Indian southwest monsoon. Copyright © 2005 John Wiley & Sons, Ltd.  相似文献   
452.
In this paper we prove the existence of ring-type bounded motion in an isolated system consisting of a massive point particle and a homogeneous cube. We study the case of planar motion where the particle moves in a symmetry plane of the cube and we use a rotating frame of reference with its center at the mass center of the cube and its axes coinciding with the symmetry axes of the cube. We prove that, for negative values of the total energy and properly chosen values of the total angular momentum, the relative distance of the bodies has an upper and a lower bound-i.e., the regions of possible motion lie inside an annulus around the cube (motion inside a ring or an island).  相似文献   
453.
454.
A regular perturbation analysis is presented for natural convection flow over an uniform flux vertical surface with temperature dependent viscosity. Numerical calculations are presented forP r=6.7 which show that the first-order correction to the local temperature difference and to the local skin-fraction are negative whereas it is positive for the local Nusselt number. The effects of variable viscosity on the temperature, velocity profiles, the local temperature difference, the local Nusselt number and the local skin fraction are discussed.  相似文献   
455.
456.
457.
458.
The muon flux at the South Pole was measured for five zenith angles, 0°, 15°, 35°, 82.13° and 85.15° with a scintillator muon telescope incorporating ice Cherenkov tank detectors as the absorber. We compare the measurements with other data and with calculations.  相似文献   
459.
It is shown by linear stability analysis that a preplanetary (presatellite) disk of dust and gas with Keplerian velocity field can become unstable due to the collective self-gravity of the disk. The radial distribution of rings, which may result from this instability, is derived. These rings later on can be the formation sites for planets around the Sun and for satellites around the planets. The derived orbits are shown to be in good agreement with that of the planets and the satellites (of Jupiter, Saturn, and Uranus). Predictions and conclusions seem to be possible for the existence of three yet unknown Uranian satellites, the origin of the early Moon and the possible radial extension of the planetary system.  相似文献   
460.
The dispersion relation for longitudinal waves in a one-dimensional ultrarelativistic plasma is calculated. Analytical and numerical results for the growth rate and frequency of the two-stream instability are presented as a function of the energy spread in the denser stream when the dilute stream is cold. The case of energy spreads in both beams is investigated numerically: it is found that relatively small energy spreads in both streams can lead to suppression of the instability.  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