全文获取类型
收费全文 | 10711篇 |
免费 | 2140篇 |
国内免费 | 3659篇 |
专业分类
测绘学 | 1250篇 |
大气科学 | 4848篇 |
地球物理 | 2217篇 |
地质学 | 3308篇 |
海洋学 | 1818篇 |
天文学 | 432篇 |
综合类 | 739篇 |
自然地理 | 1898篇 |
出版年
2024年 | 68篇 |
2023年 | 153篇 |
2022年 | 395篇 |
2021年 | 511篇 |
2020年 | 543篇 |
2019年 | 649篇 |
2018年 | 519篇 |
2017年 | 556篇 |
2016年 | 511篇 |
2015年 | 563篇 |
2014年 | 754篇 |
2013年 | 903篇 |
2012年 | 780篇 |
2011年 | 759篇 |
2010年 | 646篇 |
2009年 | 787篇 |
2008年 | 785篇 |
2007年 | 900篇 |
2006年 | 795篇 |
2005年 | 691篇 |
2004年 | 625篇 |
2003年 | 493篇 |
2002年 | 477篇 |
2001年 | 396篇 |
2000年 | 341篇 |
1999年 | 302篇 |
1998年 | 257篇 |
1997年 | 253篇 |
1996年 | 223篇 |
1995年 | 166篇 |
1994年 | 149篇 |
1993年 | 126篇 |
1992年 | 111篇 |
1991年 | 85篇 |
1990年 | 61篇 |
1989年 | 36篇 |
1988年 | 33篇 |
1987年 | 26篇 |
1986年 | 18篇 |
1985年 | 15篇 |
1984年 | 10篇 |
1983年 | 7篇 |
1982年 | 8篇 |
1981年 | 2篇 |
1980年 | 1篇 |
1979年 | 8篇 |
1978年 | 4篇 |
1977年 | 3篇 |
1976年 | 2篇 |
1954年 | 4篇 |
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
971.
采用辐照度基法对FY-1C气象卫星可见近红外通道进行绝对辐射定标 总被引:7,自引:1,他引:6
介绍另一种在轨卫星传感器绝对辐射定标——辐照度基法定标,并利用敦煌辐射校正场对FY-1C卫星可见近红外通道进行定标。通常的反射率基法定标,表观反射率计算的一个重要误差来源是对气溶胶散射的近似计算。辐照度基法定标采用实际测量的漫射与总辐射比来代替辐射传输计算的气溶胶散射。利用该方法对FY-1C卫星的5次定标结果表明,大部分日期辐照度基法和反射率基法定标结果非常吻合,肯定了辐照度基法的正确性,但在气溶胶含量较大时,辐照度基法提高定标精度的优点显现出来,能够减少辐射传输模式对气溶胶散射计算带来的误差,提高最终的绝对辐射定标精度。 相似文献
972.
The classic two-level or equivalent two-level model that includes only the statistical equilibriumof radiative and thermal processes of excitation and quenching between two vibrational energy levelsis extended by adding chemical production to the rate equations. The modifications to the non-localthermodynamic equilibrium source function and cooling rate are parameterized by φc, which characterizesthe ratio of chemical production to collisional quenching. For applications of broadband emission of O3 at9.6 μm, the non-LTE effect of chemical production on the cooling rate and limb emission is proportionalto the ratio of O to O3. For a typical [O]/[O3], the maximum enhancements of limb radiance and coolingrate are about 15%-30% and 0.03-0.05 K day-1, respectively, both occurring near the mesopause regions.This suggests that the broadband limb radiance above ~80 km is sensitive to O3 density but not sensitiveto the direct cooling rate along the line-of-sight, which makes O3 retrieval feasible but the direct coolingrate retrieval difficult by using the O3 9.6 μm band limb emission. 相似文献
973.
1997年1月21日-1998年8月27日新疆伽师发生了包含9次6级地震的强震群,震源机制解表明有NE向和NW向两个节面.有观点认为主破裂面为NNW向.本通过数字地震台阵的余震序列精确定位、震源破裂过程及滑动方向、震群空间分布图像、地震烈度等震线长轴走向和微、宏观震中动态变化方向等多种方法分析后,综合判定9次6级地震的主破裂面走向极可能为北东方向. 相似文献
974.
A remote sensing model for monitoring soil evaporation based on differential thermal inertia and its validation 总被引:2,自引:0,他引:2
To develop geosciences quantification and multi-dimensional researches will be an inevitable trend in the 21st century. The interaction between the land surface and the atmosphere not only serves as an important component in geosciences quantification, bu… 相似文献
975.
Sea surface height and transport stream function of the South China Sea from a variable-grid global ocean circulation model 总被引:8,自引:0,他引:8
The study on the South China Sea (SCS) circulation has a history of more than 40 years. Nevertheless, the SCS circulation is not fully understood compared with the Bohai Sea, Yellow Sea and East China Sea (ECS). Many numerical studies on the SCS circulati… 相似文献
976.
本文论述了“地球空间双星探测计划”(简称双星计划)及其与全球环境变化的关系。地球空间双星探测计划包括两颗小卫星,分别运行于目前国际上地球空间探测卫星尚未覆盖的近地赤道区和近地极区。双星计划的主要科学目标是用高分辨率的仪器在近地空间的主要活动区探测场和粒子的时空变化;研究磁层空间暴(磁层亚暴、磁暴和磁层粒子暴)的触发机制及其对太阳活动和行星际扰动的响应过程;建立地球空间环境的动态模式。为了实现科学目标,赤道区卫星和极区卫星上各载有8台探测仪器。近地赤道区卫星的轨道是:近地点550km左右,远地点60000km左右,倾角约28.5°;近地极区卫星的轨道是:近地点700km,远地点40000km,倾角约90°。为了使双星计划与欧洲空间局ClusterII卫星相配合,赤道区卫星计划于2003年6月发射,极区卫星计划于2003年12月发射。双星计划与ClusterII卫星相配合,可形成地球空间6点探测计划,这将成为21世纪初国际上重要的地球空间探测计划。本文概要讨论了双星计划与地球系统各圈层的关系,包括与大气圈、生物圈、地球内部各圈层及全球环境变化的关系。 相似文献
977.
The proposed existence of magnetic lineations in the Terra Cimmeria and Terra Sirenum regions of Mars was initially explained by Earth-like sea-floor spreading. Here we argue instead that these lineations could have been formed at a convergent plate margin through collision and accretion of terranes. A similar process produced banded magnetic anomalies, similar in geometry and even in size to those in Earth's North American Cordillera. Because only sparse and generally weak anomalies have been detected in the martian northern lowlands, which could constitute an analog to the terrestrial oceanic crust, it is possible that the magnetic field stopped its activity while crustal recycling was still active in Mars. 相似文献
978.
Christopher D. CooperJohn F. Mustard 《Icarus》2002,158(1):42-55
The goal of this work is to determine the spectroscopic properties of sulfate in martian soil analogs over the wavelength range 0.3 to 25 μm (which is relevant to existing and planned remotely sensed data sets for Mars). Sulfate is an abundant component of martian soil (up to 9% SO3 by weight) and apparently exists as a particulate in the soil but also as a cement. Although previous studies have addressed the spectroscopic identity of sulfates on Mars, none have used laboratory mixtures of materials with sulfates at the abundances measured by landed spacecraft, nor have any works considered the effect of salt-cementation on spectral properties of soil materials. For this work we created mixtures of a palagonitic soil (JSC Mars-1) and sulfates (MgSO4 and CaSO4·2H2O). The effects of cementation were determined and separated from the effects of packing and hydration by measuring the samples as loose powders, packed powders, cemented materials, and disaggregated materials. The results show that the presence of particulate sulfate is best observed in the 4-5 μm region. Soils cemented with sulfate exhibit a pronounced restrahlen band between 8 and 9 μm as well as well-defined absorptions in the 4-5 μm region. Cementation effects are distinct from packing effects and disaggregation of cemented samples rapidly diminishes the strength of the restrahlen bands. The results of this study show that sulfate in loose materials is more detectable in the near infrared (4-5 μm) than in the thermal infrared (8-9 μm). However, cemented materials are easily distinguished from loose mixtures in the thermal infrared because of the high values of their absorption coefficient in this region. Together these results suggest that both wavelength regions are important for determining the spatial extent and physical form of sulfates on the surface of Mars. 相似文献
979.
980.
Guillaume Favreau Christian Leduc Christelle Marlin Abdou Guéro 《Comptes Rendus Geoscience》2002,334(6):395-401
In southwest Niger, the Continental Terminal water table displays a natural hollow shape about 10 m in depth over an area of 4000 km2. A 10-year survey of this hollow aquifer has shown that current recharge is above . The water table has risen continuously since the 1950–1960s as a result of land clearance. This shows a disequilibrium in the aquifer balance. The long-term recharge rate is estimated by radioisotopes to be around . This figure fits with the only possible origin of the piezometric depression, i.e. evapotranspiration losses in its centre. To cite this article: G. Favreau et al., C. R. Geoscience 334 (2002) 395–401. 相似文献