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   252916篇
  免费   5213篇
  国内免费   3279篇
测绘学   7026篇
大气科学   18894篇
地球物理   53101篇
地质学   87837篇
海洋学   21126篇
天文学   54639篇
综合类   1002篇
自然地理   17783篇
  2021年   2164篇
  2020年   2574篇
  2019年   2829篇
  2018年   3378篇
  2017年   3108篇
  2016年   5640篇
  2015年   4192篇
  2014年   6909篇
  2013年   14226篇
  2012年   6424篇
  2011年   7715篇
  2010年   6756篇
  2009年   9381篇
  2008年   8184篇
  2007年   7566篇
  2006年   9597篇
  2005年   7633篇
  2004年   7549篇
  2003年   7048篇
  2002年   6648篇
  2001年   5946篇
  2000年   5915篇
  1999年   5197篇
  1998年   5222篇
  1997年   4979篇
  1996年   4203篇
  1995年   4292篇
  1994年   3989篇
  1993年   3741篇
  1992年   3491篇
  1991年   3518篇
  1990年   3617篇
  1989年   3321篇
  1988年   3159篇
  1987年   3703篇
  1986年   3249篇
  1985年   4114篇
  1984年   4621篇
  1983年   4298篇
  1982年   4216篇
  1981年   3845篇
  1980年   3594篇
  1979年   3432篇
  1978年   3439篇
  1977年   3212篇
  1976年   2960篇
  1975年   2900篇
  1974年   2864篇
  1973年   3058篇
  1972年   1990篇
排序方式: 共有10000条查询结果,搜索用时 26 毫秒
941.
942.
Photoionization by stars cannot be the only cause for the diffuseionized gas component in the distant halos of galaxies.Quasistationary localized magnetic reconnection can efficientlycontribute to the ionization of the extraplanar halo gas. The gas isheated and re-ionized in numerous current filaments fast enough tocompensate recombination. The necessary magnetic energy is provided bythe disk activity.  相似文献   
943.
D.L. Mickey 《Solar physics》2004,220(1):21-27
I describe a method for quickly and accurately determining the plate parallelism in a tunable Fabry-Pérot interferometer. The method takes advantage of the fact that our Fabry-Pérot is installed in a spectropolarimeter: we measure profiles of solar or telluric absorption lines in three differently polarized telescope subapertures and use the residual polarization profiles to determine the plate parallelism error. An example of the error as a function of time during the observing day is also shown; it changes in a consistent way with telescope hour angle but the drift is enough to require frequent adjustment.  相似文献   
944.
An experiment aboard the Scripps Institution of Oceanography's RV Thomas Washington has demonstrated the seafloor mapping advantages to be derived from combining the high-resolution bathymetry of a multibeam echo-sounder with the sidescan acoustic imaging plus wide-swath bathymetry of a shallow-towed bathymetric sidescan sonar. To a void acoustic interference between the ship's 12-kHz Sea Beam multibeam echo-sounder and the 11-12-kHz SeaMARC II bathymetric sidescan sonar system during simultaneous operations, Sea Beam transmit cycles were scheduled around SeaMARC II timing events with a sound source synchronization unit originally developed for concurrent single-channel seismic, Sea Beam, and 3.5-kHz profile operations. The scheduling algorithm implemented for Sea Beam plus SeaMARC II operations is discussed, and the initial results showing their combined seafloor mapping capabilities are presented  相似文献   
945.
The structure of beam noise measured at the output of a vertical array in a range dependent ocean basin was investigated using the modified wide-angle parabolic equation (PE). Noise sources were distributed throughout the basin, and the field due to each noise source at an array located in the midbasin was calculated. The response of the array to the superposition of the noise sources was found by beamforming. An efficient and direct approach that superimposes the noise sources on the PE field as the field is marched toward the array was developed. Downslope calculations of the midbasin vertical directionality were made between 50 and 400 Hz with this technique. Use of a geoacoustic model shows that the bottom behaves as a low-pass filter  相似文献   
946.
A four-year record from an inverted echo sounder deployed near Palmyra Island at 6°N in the central Pacific Ocean is compared with a simultaneous record of subsurface pressure from this island lagoon. A factor m, converting round-trip acoustic travel time to surface dynamic height relative to a deep pressure level, was estimated from the ratio of the spectra of the two records in the energetic synoptic oscillation band. Year-to-year variation in m was not statistically significant. For the overall record, m was found to be -70±8 dynamic m/s, where the error bounds represent a 90% confidence interval. This is consistent with first-baroclinic-mode excitation  相似文献   
947.
948.
949.
Astronomy Letters - The acceleration of anomalous cosmic rays (ACRs) at the heliospheric termination shock and their influence on the shock structure and location are analyzed in terms of a...  相似文献   
950.
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