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   1493篇
  免费   259篇
  国内免费   390篇
测绘学   62篇
大气科学   318篇
地球物理   351篇
地质学   787篇
海洋学   250篇
天文学   74篇
综合类   157篇
自然地理   143篇
  2024年   13篇
  2023年   22篇
  2022年   58篇
  2021年   85篇
  2020年   75篇
  2019年   63篇
  2018年   57篇
  2017年   69篇
  2016年   81篇
  2015年   60篇
  2014年   89篇
  2013年   74篇
  2012年   63篇
  2011年   84篇
  2010年   75篇
  2009年   85篇
  2008年   73篇
  2007年   60篇
  2006年   47篇
  2005年   51篇
  2004年   47篇
  2003年   47篇
  2002年   56篇
  2001年   56篇
  2000年   53篇
  1999年   82篇
  1998年   64篇
  1997年   67篇
  1996年   60篇
  1995年   46篇
  1994年   49篇
  1993年   34篇
  1992年   55篇
  1991年   26篇
  1990年   19篇
  1989年   23篇
  1988年   22篇
  1987年   13篇
  1986年   13篇
  1985年   9篇
  1984年   8篇
  1983年   5篇
  1982年   1篇
  1981年   1篇
  1979年   1篇
  1954年   1篇
排序方式: 共有2142条查询结果,搜索用时 0 毫秒
101.
Qiu  Jiong  Wang  Haimin  Chae  Jongchul  Goode  Philip R. 《Solar physics》1999,190(1-2):153-165

An active region loop system was observed in a decaying active region for three hours by TRACE and BBSO in a joint campaign on September 27, 1998. Continuous mass motion was seen in Hα offband filtergrams throughout the three hours, and some UV loops were exhibited transient brightenings. We find that: (1) cool material was flowing along the loops at a speed of at least 20 km s?1. Further, in Hα red and blue wings, we see mass motion along different loops in opposite directions. This is the first report of a counter-streaming pattern of mass motion in an Hα loop system. (2) Transient brightenings of different UV loops at different times were observed at C?iv 1550 Å. These brightened UV loops were located in the same region and at the same altitudes as the Hα loops. The observations show a clear correlation between the transient brightenings of UV loops and mass motion in Hα loops. (3) Both footpoints of the loop system were located in regions of mixed magnetic polarities. Frequent micro-flares at one footpoint of the loops with small-scale brightenings spreading along the loop leg were observed before the brightening and rising of one C?iv loop. Similar to the case of a filament, the continuous mass motion along the loops seems important for maintaining the cool Hα loop system at coronal height. There may be an indication that the mass motion in cool Hα loops and the correlated transient brightening of the active region loops were due to the small-scale chromospheric magnetic reconnection at the footpoint regions of the loop system.

  相似文献   
102.
亚洲特提斯域岩相古地理与油气聚集地质特征   总被引:7,自引:1,他引:6  
亚洲特提斯域油气在地理上主要分布于西亚段南带,其次为西亚段北带、东南亚段中带,再次为中亚段。对古、中、新特提斯域的岩相古地理特征作了分析研究,并编制了相关的岩相古地理图。认为油气分布在盆地类型上主要与前陆盆地、克拉通边缘盆地相关,盆地形态主要与台地、环形坳陷、线形坳陷等沉积—构造环境相关,其成烃物质的沉积-构造环境多位于古赤道与45°古纬度之间。提出盆地保存是盆地油气评价的先决条件。指出了亚洲特提斯域南带、中带和北带的油气勘探新领域。  相似文献   
103.
In situ measurements of stratospheric H2SO4 and HSO3vapors using passive chemical ionization mass spectrometry were made in October 1982 after the eruption of volcano El Chichon. Data were obtained between about 20 and 41 km showing [H2SO4 + HSO3] sum concentrations between about 104 and 2 × 105 cm?3 below 29 km and a steep rise above this altitude. Maximum [H2SO4 + HSO3] values of about 3 × 106 cm?3 are reached above 35 km.Partial [HSO3] concentrations increase above 34 km reaching about 4 × 105cm?3 around 40 km. From the measurements it is concluded that H2SO4 and probably HSO3photolysis have an important influence above 34 km leading to the observed increase of [HSO3] and a depletion of H2SO4vapor.It also seems that the data support the view of heterogeneous HSO3 removal. If correct, this would imply that stratospheric aerosols are formed primarily from HSO3 rather than H2SO4vapor.  相似文献   
104.
This article presents a deterministic model for sub-block-level population estimation based on the total building volumes derived from geographic information system (GIS) building data and three census block-level housing statistics. To assess the model, we generated artificial blocks by aggregating census block areas and calculating the respective housing statistics. We then applied the model to estimate populations for sub-artificial-block areas and assessed the estimates with census populations of the areas. Our analyses indicate that the average percent error of population estimation for sub-artificial-block areas is comparable to those for sub-census-block areas of the same size relative to associated blocks. The smaller the sub-block-level areas, the higher the population estimation errors. For example, the average percent error for residential areas is approximately 0.11 percent for 100 percent block areas and 35 percent for 5 percent block areas.  相似文献   
105.
以中国北方7个苹果主产省为研究区域,基于研究区域及周边100 m范围内210个气象站1970—2019年逐日气象数据和1 km分辨率的数字高程数据,采用最小湿度法对作物系数(Kc)进行逐日估算,并利用基于样条函数插值理论的专业气象插值软件ANUSPLIN对逐日气象数据进行空间插值,计算苹果各关键生育期需水量和降水适宜度。结合苹果优势主产区地理分布确定降水适宜度阈值范围。利用相关数理统计方法明确苹果需水特征和降水适宜度时空变化特征,并对苹果全生育期降水适宜性进行评价。结果表明:苹果全年平均需水量大多数区域为500.0~800.0 mm,萌芽-幼果期、果实膨大期和着色-成熟期平均需水量占全年平均需水量的比率分别为0.186~0.282,0.392~0.562和0.159~0.282。苹果全年、萌芽-幼果期、果实膨大期和着色-成熟期降水适宜度阈值范围分别为0.49~2.07,0.25~1.70,0.54~2.25和0.46~2.65。各生育阶段降水适宜度处在阈值范围内的区域分别占85.4%,87.4%,85.6%和84.9%。苹果全生育期降水的最适宜、次适宜和不适宜区分别占研究区域的31.9%,50.6%和17.5%。  相似文献   
106.
辽宁清原绿岩地层自下而上分为榆树底组、红透山组和南天门组。小莱河铁矿区榆树底组斜长角闪岩岩石化学性质和稀土元素分布曲线表明,该岩石的原岩属太古代亏损型(DAT)拉斑玄武岩。此斜长角闪岩中的角闪石的两个~(40)Ar/~(39)Ar年龄谱给出该岩石的变质作用发生在29.9亿年。清原绿岩地层形成时代可能在30亿年或稍早一些。全球范围绿岩地层的年龄是35—19亿年,峰值是27亿年.清原绿岩地层的早期形成年龄则大于全球绿岩的峰值年龄。  相似文献   
107.
108.
This paper uses the catastrophic landslide that occurred in Zhongxing Town, Dujiangyan City, as an example to study the formation mechanism of landslides induced by heavy rainfall in the post-Wenchuan earthquake area. The deformation characteristics of a slope under seismic loading were investigated via a shaking table test. The results show that a large number of cracks formed in the slope due to the tensile and shear forces of the vibrations, and most of the cracks had angles of approximately 45° with respect to the horizontal. A series of flume tests were performed to show how the duration and intensity of rainfall influence the responses of the shaken and non-shaken slopes. Wetting fronts were recorded under different rainfall intensities, and the depth of rainfall infiltration was greater in the shaken slope than in the non-shaken slope because the former experienced a greater extreme rainfall intensity under the same early rainfall and rainfall duration conditions. At the beginning of the rainfall infiltration experiment, the pore water pressure in the slope was negative, and settling occurred at the top of the slope. With increasing rainfall, the pore water pressure changed from negative to positive, and cracks were observed on the back surface of the slope and the shear outlet of the landslide on the front of the slope. The shaken slope was more susceptible to crack formation than the non-shaken slope under the same rainfall conditions. A comparison of the responses of the shaken and non-shaken slopes under heavy rainfall revealed that cracks formed by earthquakes provided channels for infiltration. Soil particles in the cracks of slopes were washed away, and the pore water pressure increased rapidly, especially the transient pore water pressure in the slope caused by short-term concentrated rainfall which decreased rock strength and slope stability.  相似文献   
109.
High-accuracy large-eddy simulations of neutral atmospheric surface-layer flow over a gapped plant canopy strip have been performed. Subgrid-scale (SGS) motions are parameterized by the Sagaut mixed length SGS model, with a modification to compute the SGS characteristic length self-adaptively. Shaw’s plant canopy model, taking the vertical variation of leaf area density into account, is applied to study the response of the atmospheric surface layer to the gapped dense forest strip. Differences in the region far away from the gap and in the middle of the gap are investigated, according to the instantaneous velocity magnitude, the zero-plane displacement, the potential temperature and the streamlines. The large-scale vortex structure, in the form of a roll vortex, is revealed in the region far away from the gap. The nonuniform spatial distribution of plants appears to cause the formation of the coherent structure. The roll vortex starts in the wake of the canopy, and results in strong fluctuations throughout the entire canopy region. Wind sweeps and ejections in the plant canopy are also attributed to the large vortex structure.  相似文献   
110.
四川盆地中二叠统栖霞组勘探发现系列油气,资源潜力巨大。但广安地区中二叠统栖霞组的岩石学特征及沉积环境研究薄弱。在野外地质调查的基础上,结合室内岩石学、岩相学等综合分析,对广安地区栖霞组碳酸盐岩岩石特征、沉积相类型及其古地理展布特征进行了系统研究。结果表明:广安地区栖霞组主要发育亮晶颗粒灰岩、亮晶生物碎屑灰岩、微晶生物碎屑灰岩、微晶颗粒灰岩、生物碎屑微晶灰岩、含生物碎屑微晶灰岩和泥晶灰岩7种岩石类型;碳酸盐岩颗粒主要以生物碎屑为主,部分层位发育球粒;古生物化石以三叶虫、腕足和有孔虫为主,同时可见棘皮类和藻类;栖霞组沉积期主要为碳酸盐岩台地沉积环境,其中栖霞组晚期(栖二段)台缘滩和台内滩较为发育,为该区油气成藏提供了有利条件。  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