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   26969篇
  免费   490篇
  国内免费   217篇
测绘学   551篇
大气科学   2026篇
地球物理   5423篇
地质学   9415篇
海洋学   2207篇
天文学   6219篇
综合类   48篇
自然地理   1787篇
  2021年   166篇
  2020年   203篇
  2019年   218篇
  2018年   504篇
  2017年   476篇
  2016年   586篇
  2015年   450篇
  2014年   623篇
  2013年   1273篇
  2012年   766篇
  2011年   1048篇
  2010年   926篇
  2009年   1279篇
  2008年   1093篇
  2007年   1113篇
  2006年   1034篇
  2005年   866篇
  2004年   881篇
  2003年   845篇
  2002年   777篇
  2001年   716篇
  2000年   665篇
  1999年   596篇
  1998年   607篇
  1997年   597篇
  1996年   460篇
  1995年   433篇
  1994年   389篇
  1993年   349篇
  1992年   324篇
  1991年   279篇
  1990年   312篇
  1989年   296篇
  1988年   240篇
  1987年   321篇
  1986年   266篇
  1985年   366篇
  1984年   395篇
  1983年   381篇
  1982年   344篇
  1981年   324篇
  1980年   324篇
  1979年   297篇
  1978年   319篇
  1977年   274篇
  1976年   275篇
  1975年   283篇
  1974年   241篇
  1973年   248篇
  1972年   168篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
51.
52.
We study the efficiency at which a black hole or dense star cluster spirals in to the Galactic Centre. This process takes place on a dynamical friction time-scale, which depends on the value of the Coulomb logarithm (ln Λ). We determine the accurate value of this parameter using the direct N -body method, a tree algorithm and a particle-mesh technique with up to two million plus one particles. The three different techniques are in excellent agreement. Our measurement for the Coulomb logarithm appears to be independent of the number of particles. We conclude that  ln Λ= 6.6 ± 0.6  for a massive point particle in the inner few parsec of the Galactic bulge. For an extended object, such as a dense star cluster, ln Λ is smaller, with a value of the logarithm argument Λ inversely proportional to the object size.  相似文献   
53.
54.
55.
56.
Non-Newtonian topographic relaxation on Europa   总被引:1,自引:0,他引:1  
F. Nimmo 《Icarus》2004,168(1):205-208
Models of topographic support on Europa by lateral shell thickness variations have previously assumed a Newtonian ice viscosity. Here I show that using a more realistic stress-dependent viscosity gives relaxation times which can be significantly different. Topography of wavelength 100 km cannot be supported by lateral shell thickness variations for ∼50 Myr, unless the shell thickness is <10 km or the ice grain size >10 mm. Shorter wavelength topography would require even thinner shells, but may be supported elastically. Global-scale variations in shell thickness, however, can be supported for geological timescales if the shell thickness is O(10 km).  相似文献   
57.
58.
59.
60.
Conclusion The above account is just a selection of Perthes' multifarious activities. As such it is fragmentary and incomplete. Many other publications and collaborators could have been mentioned. Even in its incompleteness the report may justify the statement that the success of Justus Perthes Geographische Verlagsanstalt, was apart from the managing qualities of its governors, undoubtedly due to the long series of scholarly competent collaborators whom they succeeded in engaging. As illustrated above most of theme were among the avant garde of the profession. Apparently they were at ease with Justus Perthes where they were granted enough freedom of action to realise their ambitious projects under the vigilant eye of the management. In fact the history of the firm is a continuous story of their achievements. Their combined effort initiated modern scientific atlas-making, laid down the foundation of methodic school cartography and accelerated the growth of thematic cartography. The Justus Perthes maps and atlasses stand for intellectual honestly and have an authoritative appearance of truth and exactness. For a long time to come the name of the firm will be considered as a classical example of the promotion of geography and cartography by private enterprise.  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