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291.
Stephens P Edkins S Davies H Greenman C Cox C Hunter C Bignell G Teague J Smith R Stevens C O'Meara S Parker A Tarpey P Avis T Barthorpe A Brackenbury L Buck G Butler A Clements J Cole J Dicks E Edwards K Forbes S Gorton M Gray K Halliday K Harrison R Hills K Hinton J Jones D Kosmidou V Laman R Lugg R Menzies A Perry J Petty R Raine K Shepherd R Small A Solomon H Stephens Y Tofts C Varian J Webb A West S Widaa S Yates A Brasseur F Cooper CS Flanagan AM Green A Knowles M Leung SY Looijenga LH 《Nature genetics》2005,37(6):590-592
We examined the coding sequence of 518 protein kinases, approximately 1.3 Mb of DNA per sample, in 25 breast cancers. In many tumors, we detected no somatic mutations. But a few had numerous somatic mutations with distinctive patterns indicative of either a mutator phenotype or a past exposure. 相似文献
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Golgi biogenesis in Toxoplasma gondii 总被引:7,自引:0,他引:7
Pelletier L Stern CA Pypaert M Sheff D Ngô HM Roper N He CY Hu K Toomre D Coppens I Roos DS Joiner KA Warren G 《Nature》2002,418(6897):548-552
Two models have been put forward to explain the growth of new Golgi during the cell cycle. The first suggests that a new Golgi grows out of the endoplasmic reticulum by de novo synthesis. The second suggests that a pre-existing Golgi is needed for the growth of a new one, that is, the Golgi is an autonomously replicating organelle. To resolve this issue, we have exploited the simplicity of the apicomplexan parasite Toxoplasma gondii, which has only a single Golgi stack. Here we show, by using video fluorescence microscopy and three-dimensional reconstructions of serial thin sections, that the Golgi grows by a process of lateral extension followed by medial fission. Further fission leads to the inheritance by each daughter of a pair of Golgi structures, which then coalesce to re-form a single Golgi. Our results indicate that new Golgi grow by autonomous duplication and raise the possibility that the Golgi is a paired structure that is analogous to centrioles. 相似文献
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It is generally accepted that the acute sensitivity and frequency discrimination of mammalian hearing requires active mechanical amplification of the sound stimulus within the cochlea. The prevailing hypothesis is that this amplification stems from somatic electromotility of the outer hair cells attributable to the motor protein prestin. Thus outer hair cells contract and elongate in synchrony with the sound-evoked receptor potential. But problems arise with this mechanism at high frequencies, where the periodic component of the receptor potential will be attenuated by the membrane time constant. On the basis of work in non-mammalian vertebrates, force generation by the hair bundles has been proposed as an alternative means of boosting the mechanical stimulus. Here we show that hair bundles of mammalian outer hair cells can also produce force on a submillisecond timescale linked to adaptation of the mechanotransducer channels. Because the bundle motor may ultimately be limited by the deactivation rate of the channels, it could theoretically operate at high frequencies. Our results show the existence of another force generator in outer hair cells that may participate in cochlear amplification. 相似文献
296.
One of the most important considerations when planning the next generation of ground-based optical astronomical telescopes is to choose a site that has excellent 'seeing'--the jitter in the apparent position of a star that is caused by light bending as it passes through regions of differing refractive index in the Earth's atmosphere. The best mid-latitude sites have a median seeing ranging from 0.5 to 1.0 arcsec (refs 1-5). Sites on the Antarctic plateau have unique atmospheric properties that make them worth investigating as potential observatory locations. Previous testing at the US Amundsen-Scott South Pole Station has, however, demonstrated poor seeing, averaging 1.8 arcsec (refs 6, 7). Here we report observations of the wintertime seeing from Dome C (ref. 8), a high point on the Antarctic plateau at a latitude of 75 degrees S. The results are remarkable: the median seeing is 0.27 arcsec, and below 0.15 arcsec 25 per cent of the time. A telescope placed at Dome C would compete with one that is 2 to 3 times larger at the best mid-latitude observatories, and an interferometer based at this site could work on projects that would otherwise require a space mission. 相似文献
297.
Stephens P Hunter C Bignell G Edkins S Davies H Teague J Stevens C O'Meara S Smith R Parker A Barthorpe A Blow M Brackenbury L Butler A Clarke O Cole J Dicks E Dike A Drozd A Edwards K Forbes S Foster R Gray K Greenman C Halliday K Hills K Kosmidou V Lugg R Menzies A Perry J Petty R Raine K Ratford L Shepherd R Small A Stephens Y Tofts C Varian J West S Widaa S Yates A Brasseur F Cooper CS Flanagan AM Knowles M Leung SY Louis DN Looijenga LH Malkowicz B Pierotti MA Teh B Chenevix-Trench G 《Nature》2004,431(7008):525-526
The protein-kinase family is the most frequently mutated gene family found in human cancer and faulty kinase enzymes are being investigated as promising targets for the design of antitumour therapies. We have sequenced the gene encoding the transmembrane protein tyrosine kinase ERBB2 (also known as HER2 or Neu) from 120 primary lung tumours and identified 4% that have mutations within the kinase domain; in the adenocarcinoma subtype of lung cancer, 10% of cases had mutations. ERBB2 inhibitors, which have so far proved to be ineffective in treating lung cancer, should now be clinically re-evaluated in the specific subset of patients with lung cancer whose tumours carry ERBB2 mutations. 相似文献
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