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   44882篇
  免费   1386篇
  国内免费   1033篇
测绘学   1091篇
大气科学   3533篇
地球物理   9482篇
地质学   16298篇
海洋学   4064篇
天文学   9174篇
综合类   267篇
自然地理   3392篇
  2022年   302篇
  2021年   542篇
  2020年   560篇
  2019年   624篇
  2018年   1089篇
  2017年   1047篇
  2016年   1258篇
  2015年   896篇
  2014年   1270篇
  2013年   2306篇
  2012年   1589篇
  2011年   2149篇
  2010年   1900篇
  2009年   2434篇
  2008年   2041篇
  2007年   2129篇
  2006年   2006篇
  2005年   1475篇
  2004年   1386篇
  2003年   1298篇
  2002年   1217篇
  2001年   1014篇
  2000年   1032篇
  1999年   817篇
  1998年   860篇
  1997年   814篇
  1996年   707篇
  1995年   684篇
  1994年   592篇
  1993年   512篇
  1992年   510篇
  1991年   451篇
  1990年   546篇
  1989年   443篇
  1988年   434篇
  1987年   516篇
  1986年   422篇
  1985年   535篇
  1984年   658篇
  1983年   564篇
  1982年   549篇
  1981年   463篇
  1980年   467篇
  1979年   416篇
  1978年   407篇
  1977年   398篇
  1976年   365篇
  1975年   357篇
  1974年   362篇
  1973年   407篇
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
71.
72.
We examine the potential contamination of cometary nuclei through impacts from asteroidal origin meteoroids. The paper uses a simple model and has the goal of determining whether asteroidal contamination is potentially significant. We assume a meteoroid power law mass distribution with index values in the range from s=1.83 to s=2.09. We used maximum and minimum models which we believe will bracket the true meteoroid mass distribution. We identify those comets which are expected to be most significantly contaminated, and find values of up to 3.6 kg of asteroidal meteoroid impact per square meter of the cometary surface per orbital revolution. This is less than the expected mass loss per perihelion passage for most comets. Therefore any remnant effects of the contamination will depend on the penetration depth of the meteoroids in the cometary nucleus, and possibly on the distribution of active and inactive areas on cometary nuclei. We present a simple model which suggests that even small meteoroids will embed relatively deeply into a cometary nucleus.  相似文献   
73.
介绍应用于美国凤凰计划的Allen望远镜阵(ATA)的对数周期馈源(LPA)概况,初步给出此种馈源的基本参数及性能,仿真估算了其驻波比和方向图,并结合正在进行中的我国500m孔径球面射电望远镜(FAST)计划,探讨了应用这种宽带馈源的可能性及其限制。  相似文献   
74.
The experimental data obtained in transit observations of the extrasolar planet HD 209458b and their comparison with theoretical inferences have led to the conclusions that HD 209458b (and other similar hot jupiters) is of a (mainly) hydrogen nature and that these objects probably possess strong magnetic fields. The results of the studies of HD 209458b and prospects for searches for the transits of other extrasolar planets are considered in detail.  相似文献   
75.
Jets and cores in Active Galactic Nuclei (AGN) constitute the dominant radio structural pattern in a broad range of angular scales from hundreds of arc seconds down to sub-milliarcseconds. This brief review desribes some recent results in studying the most compact `core-jet' morphologies in AGN using Very Long Baseline Interferometry (VLBI) technique. They include measurements of the cross-section brightness distribution in pc-scale radio jets and attempts to investigate the most compact cores with brightness temperatures in excess of 1013 K.  相似文献   
76.
77.
78.
79.
Moroz  L. V.  Baratta  G.  Distefano  E.  Strazzulla  G.  Starukhina  L. V.  Dotto  E.  Barucci  M. A. 《Earth, Moon, and Planets》2003,92(1-4):279-289
Trans-Neptunian Objects (TNOs) and Centaurs show remarkable colour variationsin the visual and near-infrared spectral regions. Surface alteration processes such asspace weathering (e.g., bombardment with ions) and impact resurfacingmay play an important role in the colour diversity of such bodies. Ion irradiation ofhydrocarbon ices and their mixtures with water ice transforms neutral (grey) surfacecolours of ices to red and further to grey. Along with the ices, TNOs and Centaursprobably contain complex carbonaceous compounds, in particular, complexhydrocarbons. Unlike ices, such refractory organic materials have originally lowvisual albedos and red colours in the visible and near-infrared ranges. Here wepresent the first results of ion irradiation experiments on asphaltite. Asphaltite isa natural complex hydrocarbon material. The reflectance spectra of asphaltite inthe 0.4–0.8 μm range have been recorded before irradiation and after eachirradiation step. We demonstrate that irradiation of this red dark material with30 keV H+ and 15 keV N+ ions gradually transforms its colour from redto grey as a result of carbonization. A moderate increase in the visual albedo hasbeen observed. These results may imply that the surfaces of primitive red objectsoptically dominated by complex refractory organics may show a similar spaceweathering trend. Our laboratory results were compared with published coloursof TNOs and Centaurs. A broad variety of spectral colours observed for TNOs andCentaurs may be reproduced by various spectra of irradiated organics correspondingto different ion fluences. However, such objects probably also contain ices and silicatecomponents which show different space weathering trends. This fact, together with alack of information about albedos, may explain difficulties to reveal correlations between surface colours within TNO and Centaur populations and their other properties, such as absolute magnitudes and orbital parameters.  相似文献   
80.
We investigate the role of seasonal variations of Titan’s stratospheric composition on the temperature. We use a general circulation model coupled with idealized chemical tracers that reproduce variations of ethane (C2H6), acetylene (C2H2), and hydrogen cyanide (HCN). Enhancement of the mole fractions of these compounds, at high latitudes in the winter hemisphere relative to their equatorial values, induces a relative decrease in temperature above approximately 0.2 mbar, with a peak amplitude around −20 K, and a relative increase in temperature below, around 1 mbar, with a peak amplitude around +7 K. These thermal effects are mainly due to the variations of the cooling to space induced by the varying distributions. The ethane, acetylene, and hydrogen cyanide variations affect the cooling rates in a similar way, with the dominant effect being due to ethane, though its latitudinal variations are small.  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