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   112017篇
  免费   2228篇
  国内免费   1406篇
测绘学   2962篇
大气科学   8639篇
地球物理   22352篇
地质学   41126篇
海洋学   9541篇
天文学   23573篇
综合类   483篇
自然地理   6975篇
  2021年   727篇
  2020年   818篇
  2019年   903篇
  2018年   4203篇
  2017年   4026篇
  2016年   3503篇
  2015年   1612篇
  2014年   2209篇
  2013年   4667篇
  2012年   3466篇
  2011年   5881篇
  2010年   5341篇
  2009年   6508篇
  2008年   5493篇
  2007年   5865篇
  2006年   3730篇
  2005年   3407篇
  2004年   3324篇
  2003年   3153篇
  2002年   2810篇
  2001年   2356篇
  2000年   2312篇
  1999年   1947篇
  1998年   1969篇
  1997年   1914篇
  1996年   1639篇
  1995年   1583篇
  1994年   1415篇
  1993年   1307篇
  1992年   1236篇
  1991年   1086篇
  1990年   1322篇
  1989年   1130篇
  1988年   1015篇
  1987年   1242篇
  1986年   1069篇
  1985年   1320篇
  1984年   1567篇
  1983年   1452篇
  1982年   1342篇
  1981年   1283篇
  1980年   1163篇
  1979年   1091篇
  1978年   1115篇
  1977年   1049篇
  1976年   979篇
  1975年   926篇
  1974年   946篇
  1973年   957篇
  1972年   573篇
排序方式: 共有10000条查询结果,搜索用时 640 毫秒
601.
602.
603.
604.
605.
The Mangala Valles system is an ∼ ∼900 km fluvially carved channel system located southwest of the Tharsis rise and is unique among the martian outflow channels in that it heads at a linear fracture within the crust as opposed to a collapsed region of chaos as is the case with the circum-Chryse channels. Mangala Valles is confined within a broad, north–south trending depression, and begins as a single valley measuring up to 350 km wide that extends northward from a Memnonia Fossae graben, across the southern highlands toward the northern lowlands. Approximately 600 km downstream, this single valley branches into multiple channels, which ultimately lose their expression at the dichotomy boundary. Previous investigations of Mangala Vallis suggested that many of the units mapped interior to the valley were depositional, related to flooding, and that a minimum of two distinct periods of flooding separated by tens to hundreds of millions of years were required to explain the observed geology. We use infrared and visible images from the THermal EMission Imaging System (THEMIS), and topographic data from the Mars Orbiting Laser Altimeter (MOLA), to investigate the nature of the units mapped within Mangala Vallis. We find that the geomorphology of the units, as well as their topographic and geographic distribution, are consistent with most of them originating from a single assemblage of volcanic flow deposits, once continuous with volcanic flows to the south of the Memnonia Fossae source graben. These flows resurfaced the broad, north–south trending depression into which Mangala Vallis formed prior to any fluvial activity. Later flooding scoured and eroded this volcanic assemblage north of the Mangala source graben, resulting in the present distribution of the units within Mangala Vallis. Additionally, our observations suggest that a single period of catastrophic flooding, rather than multiple periods separated by tens to hundreds of millions of years, is consistent with and can plausibly explain the interior geology of Mangala Vallis. Further, we present a new scenario for the source and delivery of water to the Mangala source graben that models flow of groundwater through a sub-cryosphere aquifer and up a fracture that cracks the cryosphere and taps this aquifer. The results of our model indicate that the source graben, locally enlarged to a trough near the head region of Mangala, would have required less than several days to fill up prior to any spill-over of water to the north. Through estimates of the volume of material missing from Mangala (13,000–20,000 km3), and calculation of mean discharge rates through the channel system (∼ ∼5 × 106 m3 s−1), we estimate that the total duration of fluvial activity through the Mangala Valles was 1–3 months.  相似文献   
606.
607.
608.
During a campaign of optical observations at high latitude, a bi-dimensional study of the wave structure of the OH layer has been performed in December 1981 from Sodankyla (Finland). This site is one of the three stations of the EISCAT ionosphere sounding system. It has been found that a wave field covering an area of 1 million km2 may extend to latitudes as high as 70°N. The OH wave structure shows many similarities with noctilucent clouds. The fairly large horizontal wavelength, of the order of 40 km cannot easily be explained by a wave motion at an interface. The observed wave structure seems to be a result of the propagation of an internal gravity wave in the 80–100 km region. This wave structure was often recorded during the same time as an active aurora was present. As a result, it appears that the perturbation might be correlated with particle precipitations at auroral latitudes.  相似文献   
609.
Variables related to urban park awareness are identified and methods for relaxing assumptions of perfect information in park use models are discussed. Park awareness is related to park characteristics (age and degree of development of the park), population characteristics (race, age, length of residence, recreation participation), and distance. Park attributes are stronger predictors of both park awareness and use than is distance. These findings parallel similar research on the cognitive aspects of shopping decisions.  相似文献   
610.
J. Teemu T. Mäkinen 《Icarus》2005,177(1):269-279
As a part of a project to study the cometary particle environment, a self-consistent ballistic rigid body particle colliding simulator, capable of producing fractal aggregates of icy particles modelled by hard or soft (metaball) spheres has been developed, to be used for creating test particles in future statistical studies of the cometary coma-particle interaction. Instead of a predefined sticking probability, actual surface interactions are modelled and a method for calculating internal stresses and fragmentation of an aggregate during the accretion phase is described. Simulations suggest that taking fragmentation into account has two major consequences, increase in the fractal dimension of resulting particles and a noticeable change in the mass spectrum of an ensemble.  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