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   139941篇
  免费   2295篇
  国内免费   2021篇
测绘学   4239篇
大气科学   10185篇
地球物理   28166篇
地质学   52580篇
海洋学   11352篇
天文学   27898篇
综合类   2467篇
自然地理   7370篇
  2022年   661篇
  2021年   1175篇
  2020年   1284篇
  2019年   1336篇
  2018年   8014篇
  2017年   7217篇
  2016年   6381篇
  2015年   2327篇
  2014年   3525篇
  2013年   6014篇
  2012年   4863篇
  2011年   8083篇
  2010年   6853篇
  2009年   8292篇
  2008年   7127篇
  2007年   7679篇
  2006年   4457篇
  2005年   3847篇
  2004年   3909篇
  2003年   3707篇
  2002年   3305篇
  2001年   2742篇
  2000年   2653篇
  1999年   2070篇
  1998年   2221篇
  1997年   2049篇
  1996年   1747篇
  1995年   1736篇
  1994年   1513篇
  1993年   1352篇
  1992年   1321篇
  1991年   1219篇
  1990年   1358篇
  1989年   1124篇
  1988年   1080篇
  1987年   1241篇
  1986年   1089篇
  1985年   1340篇
  1984年   1484篇
  1983年   1352篇
  1982年   1317篇
  1981年   1172篇
  1980年   1085篇
  1979年   1012篇
  1978年   1013篇
  1977年   885篇
  1976年   847篇
  1975年   830篇
  1974年   792篇
  1973年   785篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
11.
12.
We present our spectroscopic observations of the novae V1425, V1493, and V1494 Aql carried out with the 125-cm telescope at the Crimean Station of the Sternberg Astronomical Institute in the wavelength range 4000–11000 Å. We measured the emission-line intensities, determined the nova shell expansion velocities from the line profile FWHMs and components, and estimated the interstellar reddening from the first members of the Balmer series. The chemical composition of the nova shells is analyzed. Nitrogen and oxygen were found to be overabundant in V1425 and V1494 Aql; the helium abundance turned out to be normal in the two stars.  相似文献   
13.
The magnetic-field distribution outside a flat, infinitely conductive unbounded disk in the field of a point magnetic dipole is determined. A relationship is established between the problem of magnetic-field determination and the problem of the flow of an ideal incompressible fluid around an infinitely thin disk.  相似文献   
14.
15.
16.
The effects of natural fish oil,DHA oil and soybean lecithin in microparticulate diets on stress tolerance of larval gilthead seabream(Sparus aurata)were investigated after 15 days feeding trials.The tolerance of larval gilthead seabream to various stress factors such as exposure to air(lack of dissolved oxygen),changes in water temperature(low)and salinity(high) were determined.This study showed that microparticulate diet with natural fish oil and soybean lecithin was the most effective for in-creasing the tolerance of larval gilthead seabream to various stresses,and that microparticulate diet with natural fish oil and palmitic acid(16:0)was more effective than microparticulate diet with DHA oil and soybean lecithin.  相似文献   
17.
Paul Withers  S.W Bougher 《Icarus》2003,164(1):14-32
Mars Global Surveyor accelerometer observations of the martian upper atmosphere revealed large variations in density with longitude during northern hemisphere spring at altitudes of 130-160 km, all latitudes, and mid-afternoon local solar times (LSTs). This zonal structure is due to tides from the surface. The zonal structure is stable on timescales of weeks, decays with increasing altitude above 130 km, and is dominated by wave-3 (average amplitude 22% of mean density) and wave-2 (18%) harmonics. The phases of these harmonics are constant with both altitude and latitude, though their amplitudes change significantly with latitude. Near the South Pole, the phase of the wave-2 harmonic changes by 90° with a change of half a martian solar day while the wave-3 phase stays constant, suggesting diurnal and semidiurnal behaviour, respectively. We use a simple application of classical tidal theory to identify the dominant tidal modes and obtain results consistent with those of General Circulation Models. Our method is less rigorous, but simpler, than the General Circulation Models and hence complements them. Topography has a strong influence on the zonal structure.  相似文献   
18.
19.
The dynamics of co-orbital motion in the restricted three-body problem are investigated by symplectic mappings. Analytical and semi-numerical mappings have been developed and studied in detail. The mappings have been tested by numerical integration of the equations of motion. These mappings have been proved to be useful for a quick determination of the phase space structure reflecting the main characteristics of the dynamics of the co-orbital problem.  相似文献   
20.
Clear signature of non-gyrotropic energetic electron distributions was found by ISEE 1 and ISEE 2 spacecrafts just upstream of the Earth's bow shock and recently detected by in situ observations of the WIND plasma experiment. On the other hand, the appearance of non-gyrotropic ion velocity distributions is well established in the magnetotail providing evidence of magnetic reconnection processes. Motivated by these findings we introduce an analytical representation of non-Maxwellian/non-gyrotropic distribution functions, accurately fitting the characteristics of observations, where Maxwellians are recovered as special case of these highly general velocity space distributions. In particular, the analytical distribution function model can serve as basis of detailed wave-particle interaction analysis and of studies of the physical background of the evolution of both, non-gyrotropic electron and ion distributions, which is discussed for various space plasma environments.  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