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   262篇
  免费   0篇
教育与普及   3篇
理论与方法论   2篇
现状及发展   11篇
研究方法   33篇
综合类   213篇
  2012年   10篇
  2011年   20篇
  2010年   2篇
  2009年   1篇
  2008年   13篇
  2007年   16篇
  2006年   14篇
  2005年   18篇
  2004年   15篇
  2003年   20篇
  2002年   15篇
  2001年   12篇
  2000年   22篇
  1999年   3篇
  1995年   1篇
  1994年   1篇
  1993年   1篇
  1992年   4篇
  1991年   3篇
  1989年   2篇
  1979年   1篇
  1977年   1篇
  1972年   1篇
  1971年   7篇
  1970年   12篇
  1960年   2篇
  1959年   4篇
  1958年   9篇
  1957年   6篇
  1956年   6篇
  1955年   4篇
  1954年   4篇
  1948年   12篇
排序方式: 共有262条查询结果,搜索用时 15 毫秒
71.
An SNP map of human chromosome 22   总被引:35,自引:0,他引:35  
The human genome sequence will provide a reference for measuring DNA sequence variation in human populations. Sequence variants are responsible for the genetic component of individuality, including complex characteristics such as disease susceptibility and drug response. Most sequence variants are single nucleotide polymorphisms (SNPs), where two alternate bases occur at one position. Comparison of any two genomes reveals around 1 SNP per kilobase. A sufficiently dense map of SNPs would allow the detection of sequence variants responsible for particular characteristics on the basis that they are associated with a specific SNP allele. Here we have evaluated large-scale sequencing approaches to obtaining SNPs, and have constructed a map of 2,730 SNPs on human chromosome 22. Most of the SNPs are within 25 kilobases of a transcribed exon, and are valuable for association studies. We have scaled up the process, detecting over 65,000 SNPs in the genome as part of The SNP Consortium programme, which is on target to build a map of 1 SNP every 5 kilobases that is integrated with the human genome sequence and that is freely available in the public domain.  相似文献   
72.
73.
74.
Proteomics for the pore   总被引:7,自引:0,他引:7  
Blobel G  Wozniak RW 《Nature》2000,403(6772):835-836
  相似文献   
75.
Models of Jupiter's formation and structure predict that its atmosphere is enriched in oxygen, relative to the Sun, and that consequently water clouds should be present globally near the 5-bar pressure level. Past attempts to confirm these predictions have led to contradictory results; in particular, the Galileo probe revealed a very dry atmosphere at the entry site, with no significant clouds at depths exceeding the 2-bar level. Although the entry site was known to be relatively cloud-free, the contrast between the observed local dryness and the expected global wetness was surprising. Here we analyse near-infrared (around 5 microm) observations of Jupiter, a spectral region that can reveal the water vapour abundance and vertical cloud structure in the troposphere. We find that humid and extremely dry regions exist in close proximity, and that some humid regions are spatially correlated with bright convective clouds extending from the deep water clouds to the visible atmosphere.  相似文献   
76.
77.
78.
79.
80.
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