全文获取类型
收费全文 | 45743篇 |
免费 | 7313篇 |
国内免费 | 11596篇 |
专业分类
测绘学 | 5619篇 |
大气科学 | 8808篇 |
地球物理 | 8451篇 |
地质学 | 18438篇 |
海洋学 | 7076篇 |
天文学 | 5496篇 |
综合类 | 3111篇 |
自然地理 | 7653篇 |
出版年
2024年 | 168篇 |
2023年 | 574篇 |
2022年 | 1585篇 |
2021年 | 1807篇 |
2020年 | 1995篇 |
2019年 | 2354篇 |
2018年 | 1889篇 |
2017年 | 2152篇 |
2016年 | 2193篇 |
2015年 | 2463篇 |
2014年 | 2959篇 |
2013年 | 3202篇 |
2012年 | 3084篇 |
2011年 | 3286篇 |
2010年 | 2818篇 |
2009年 | 3335篇 |
2008年 | 3253篇 |
2007年 | 3365篇 |
2006年 | 3132篇 |
2005年 | 2731篇 |
2004年 | 2395篇 |
2003年 | 2073篇 |
2002年 | 1737篇 |
2001年 | 1463篇 |
2000年 | 1386篇 |
1999年 | 1240篇 |
1998年 | 1027篇 |
1997年 | 818篇 |
1996年 | 747篇 |
1995年 | 694篇 |
1994年 | 630篇 |
1993年 | 540篇 |
1992年 | 345篇 |
1991年 | 301篇 |
1990年 | 206篇 |
1989年 | 156篇 |
1988年 | 130篇 |
1987年 | 74篇 |
1986年 | 56篇 |
1985年 | 60篇 |
1984年 | 43篇 |
1983年 | 21篇 |
1982年 | 29篇 |
1981年 | 23篇 |
1980年 | 20篇 |
1979年 | 17篇 |
1978年 | 17篇 |
1977年 | 20篇 |
1976年 | 11篇 |
1954年 | 10篇 |
排序方式: 共有10000条查询结果,搜索用时 93 毫秒
101.
K. Nagamine † M. Fukugita R. Cen J.P. Ostriker 《Monthly notices of the Royal Astronomical Society》2001,327(1):L10-L14
The luminosity function of galaxies is derived from a cosmological hydrodynamic simulation of a Λ cold dark matter universe with the aid of a stellar population synthesis model. At , the resulting B -band luminosity function has a flat faint-end slope of with the characteristic luminosity and the normalization in fair agreement with observations, while the dark matter halo mass function is steep with a slope of . The colour distribution of galaxies also agrees well with local observations. We also discuss the evolution of the luminosity function, and the colour distribution of galaxies from to 5. A large evolution of the characteristic mass in the stellar mass function as a result of number evolution is compensated by luminosity evolution; the characteristic luminosity increases only by 0.8 mag from to 2, and then declines towards higher redshift, while the B -band luminosity density continues to increase from to 5 (but only slowly at . 相似文献
102.
The analyses of X-ray emission from classical novae during the outburst stage have shown that the soft X-ray emission below 1 keV, which is thought to originate from the photosphere of the white dwarf, is inconsistent with the simple blackbody model of emission. Thus, ROSAT Position Sensitive Proportional Counter (PSPC) archival data of the classical Nova Mus 1983 (GQ Mus) have been re-analysed in order to understand the spectral development in the X-ray wavelengths during the outburst stage. The X-ray spectra are fitted with the hot white dwarf (WD) atmosphere emission models developed for the remnants of classical novae near the Eddington luminosity. The post-outburst X-ray spectra of the remnant white dwarf are examined in the context of evolution on the Hertzsprung–Russell diagram using C–O enhanced atmosphere models. The data obtained in 1991 August (during the ROSAT All Sky Survey) indicate that the effective temperature is . The 1992 February data show that the white dwarf had reached an effective temperature in the range with an unabsorbed X-ray flux (i.e. ∼ bolometric flux) between and . We show that the H burning at the surface of the WD had most likely ceased at the time of the X-ray observations. Only the 1991 August data show evidence for ongoing H burning. 相似文献
103.
本文应用了最新取得的“五统一”区域重力成果,并经过对浅表松散槽(如下辽河断陷,大岩体等)的密度亏损进行补偿改正后,求取了全省的区域重力场及其垂向二次导数,计算了莫氏面等深度图。在分析区域重力场及其垂向二次导数异常特征和莫氏面起伏特征的基础上,划分出辽宁深部构造的基本格局。从平面上探讨了深部构造与地形地势、地质构造及矿产分布的关系,从剖面上剖析了辽宁省地壳分层的宏观特征 相似文献
104.
探讨用遗传算法对数学模型进行优化。考虑到控制系统稳健性的要求 ,用遗传算法寻找出控制系统最佳稳定域 ,实现控制系统数学模型的寻优。阐述了用遗传算法求解问题的步骤和参数的取值 ,并用仿真实验对优化结果进行了检验。结果表明 :在控制系统数学模型的优化中 ,遗传算法具有其他算法无可比拟的优越性。 相似文献
105.
106.
Northern Hemispheric“polar lows”,i.e.maritime,small,but fairly intense cyclonic systems have been studied formore than two decades.Recently researchers have turned their attention towards the occurrence of polar lows and othersmall-scale cyclonic disturbances on the Southern Hemisphere.In this paper a short account of our present knowledgeof Northern Hemispheric polar lows will be given,followed by some preliminary results of an investigation of the natureand occurrence of polar lows on the Southern Hemisphere. 相似文献
107.
当前,由于缺乏对气象服务投入量与产出量准确而完整的统计,要对气象服务的各种经济效益作出总体评价是困难的。然而,在专项气象服务中,却不乏原始、完整而准确的资料。作者从此出发,讨论了专项气象服务经济效益评价的理论。并通过实地调查,以彭州市气象局几项专项气象服务为例探讨了评价技术。 相似文献
108.
冰雹云雷达回波自动识别系统 总被引:2,自引:0,他引:2
利用CAPPI资料对立体风暴进行识别,计算并提供出实用的风暴结构参数,采用矩心踊跃法和矩不变量法相结合对单体风暴和混合性风暴回波进行跟踪;最小二第线性外推预报;根据WSD-88D的冰雹算法,在风暴结构基础上本文建立了Windows98操作平台上冰雹识别系统,经单站1年11次强对流天气过程的资料检验,结果表明:雹云识别精度达82%。系统建立了大量人机对话框以方便用户,增加实用性及推广性。 相似文献
109.
Based on the Intensive Field Campaign(IFC-1)data of Boreal Ecosystem-Atmosphere Study(BOREAS).a three-dimensional meso-β scale model is used to simulate the effect of boreal forests onthe lower atmosphere.A fine horizontal resolution of 2 km×2 km is used in order to distinguish thevegetative heterogeneity in the boreal region.A total of 20×25 grid points cover the entire sub-modeling area in BOREAS' South Study Area(SSA).The ecosystem types and their coverage ineach grid square are extracted from the North American Land Cover Characteristics Data Base(NALCCD)generated by the U.S.Geographical Survey(USGS)and the University of Nebraska-Lincoln(UNL).The topography of the study area is taken from the Digital Elevation Map(DEM)of USGS.The model outputs include the components of the energy balance budget within the canopyand at the ground.the turbulence parameters in the atmospheric boundary layer and the wind.temperature and humidity profiles extending up to a height of 1500 m.In addition to the fine timeand spatial step,the unique feature of the present model is the incorporation of both dynamic andbiological effects of the Boreal forest into the model parameterization scheme.The model resultscompare favorably with BOREAS' IFC-1 data in 1994 when the forest was in the luxuriant growingperiod. 相似文献
110.
T.D. Thoroughgood V.S. Dhillon S.P. Littlefair T.R. Marsh D.A. Smith 《Monthly notices of the Royal Astronomical Society》2001,327(4):1323-1333
We present spectroscopy of the eclipsing recurrent nova U Sco. The radial velocity semi-amplitude of the primary star was found to be from the motion of the wings of the He ii λ 4686-Å emission line. By detecting weak absorption features from the secondary star, we find its radial velocity semi-amplitude to be . From these parameters, we obtain a mass of for the white dwarf primary star and a mass of for the secondary star. The radius of the secondary is calculated to be , confirming that it is evolved. The inclination of the system is calculated to be , consistent with the deep eclipse seen in the light-curves. The helium emission lines are double-peaked, with the blueshifted regions of the disc being eclipsed prior to the redshifted regions, clearly indicating the presence of an accretion disc. The high mass of the white dwarf is consistent with the thermonuclear runaway model of recurrent nova outbursts, and confirms that U Sco is the best Type Ia supernova progenitor currently known. We predict that U Sco is likely to explode within ∼700 000 yr. 相似文献