全文获取类型
收费全文 | 2911篇 |
免费 | 526篇 |
国内免费 | 694篇 |
专业分类
测绘学 | 113篇 |
大气科学 | 573篇 |
地球物理 | 822篇 |
地质学 | 1533篇 |
海洋学 | 325篇 |
天文学 | 187篇 |
综合类 | 254篇 |
自然地理 | 324篇 |
出版年
2024年 | 20篇 |
2023年 | 68篇 |
2022年 | 117篇 |
2021年 | 145篇 |
2020年 | 111篇 |
2019年 | 132篇 |
2018年 | 147篇 |
2017年 | 122篇 |
2016年 | 145篇 |
2015年 | 152篇 |
2014年 | 160篇 |
2013年 | 159篇 |
2012年 | 159篇 |
2011年 | 159篇 |
2010年 | 128篇 |
2009年 | 175篇 |
2008年 | 151篇 |
2007年 | 126篇 |
2006年 | 126篇 |
2005年 | 115篇 |
2004年 | 86篇 |
2003年 | 80篇 |
2002年 | 59篇 |
2001年 | 85篇 |
2000年 | 107篇 |
1999年 | 159篇 |
1998年 | 122篇 |
1997年 | 142篇 |
1996年 | 115篇 |
1995年 | 80篇 |
1994年 | 104篇 |
1993年 | 81篇 |
1992年 | 56篇 |
1991年 | 35篇 |
1990年 | 51篇 |
1989年 | 27篇 |
1988年 | 30篇 |
1987年 | 18篇 |
1986年 | 15篇 |
1985年 | 11篇 |
1984年 | 8篇 |
1983年 | 7篇 |
1982年 | 13篇 |
1981年 | 6篇 |
1980年 | 4篇 |
1979年 | 5篇 |
1978年 | 1篇 |
1976年 | 1篇 |
1965年 | 1篇 |
1958年 | 5篇 |
排序方式: 共有4131条查询结果,搜索用时 15 毫秒
401.
基于MODIS资料的贵州植被叶面积指数的时空变化及其对气候的响应 总被引:2,自引:1,他引:1
利用2000~2006年MODIS(Moderate Resolution Imaging Spectroradiometer)卫星遥感观测的植被叶面积指数月平均资料以及相应时段的月平均气温、降水的观测资料对贵州植被的时空变化进行了分析.结果表明贵州2000~2006年植被分布受水热条件控制表现出对气候因子不同的响应关系,其中对降水的响应关系比气温明显,特别是冬季和春季,而植被在夏季和秋季的分布主要受气温的制约,与降水的关系并不明显.从季节和年际尺度的时间变化角度而言,植被对气温的响应比对降水明显,季节变化和年际变化的相关系数分别为0.89和0.73(分别通过99.9%和95%信度检验). 相似文献
402.
淮北地区一次连续性暴雨的成因分析 总被引:3,自引:1,他引:2
利用各种常规资料,分析了2005年7月7-10日发生在淮北大面积连续暴雨、大暴雨天气过程的环流背景、发生机制及成因.本次大面积连续性暴雨的天气形势为两槽一脊型,旺盛的水汽在冷空气促发下形成了强烈的上升运动,中低层有很强的切变和暖湿平流,从而不断生成中尺度对流云团.此次移动性暴雨过程的前期由不断向东移动发展的MCS造成,后期降水则由低涡切变线产生的中尺度低涡引起.冷空气不断补充南下,副高西伸至淮河以南地区,冷暖空气在淮北地区交汇,且切变线稳定少动,是此次连续性强降水产生的主要因素. 相似文献
403.
Large-Eddy Simulation of Flows over Random Urban-like Obstacles 总被引:2,自引:2,他引:0
Further to our previous large-eddy simulation (LES) of flow over a staggered array of uniform cubes, a simulation of flow
over random urban-like obstacles is presented. To gain a deeper insight into the effects of randomness in the obstacle topology,
the current results, e.g. spatially-averaged mean velocity, Reynolds stresses, turbulence kinetic energy and dispersive stresses,
are compared with our previous LES data and direct numerical simulation data of flow over uniform cubes. Significantly different
features in the turbulence statistics are observed within and immediately above the canopy, although there are some similarities
in the spatially-averaged statistics. It is also found that the relatively high pressures on the tallest buildings generate
contributions to the total surface drag that are far in excess of their proportionate frontal area within the array. Details
of the turbulence characteristics (like the stress anisotropy) are compared with those in regular roughness arrays and attempts
to find some generality in the turbulence statistics within the canopy region are discussed. 相似文献
404.
Air–sea interaction over ocean fronts and eddies 总被引:1,自引:0,他引:1
R.J. Small S.P. deSzoeke S.P. Xie L. ONeill H. Seo Q. Song P. Cornillon M. Spall S. Minobe 《Dynamics of Atmospheres and Oceans》2008,45(3-4):274
Air–sea interaction at ocean fronts and eddies exhibits positive correlation between sea surface temperature (SST), wind speed, and heat fluxes out of the ocean, indicating that the ocean is forcing the atmosphere. This contrasts with larger scale climate modes where the negative correlations suggest that the atmosphere is driving the system. This paper examines the physical processes that lie behind the interaction of sharp SST gradients and the overlying marine atmospheric boundary layer and deeper atmosphere, using high resolution satellite data, field data and numerical models. The importance of different physical mechanisms of atmospheric response to SST gradients, such as the effect of surface stability variations on momentum transfer, pressure gradients, secondary circulations and cloud cover will be assessed. The atmospheric response is known to create small-scale wind stress curl and divergence anomalies, and a discussion of the feedback of these features onto the ocean will also be presented. These processes will be compared and contrasted for different regions such as the Equatorial Front in the Eastern Pacific, and oceanic fronts in mid-latitudes such as the Gulf Stream, Kuroshio, and Agulhas Return Current. 相似文献
405.
2009年10月底到11月底,包括北京在内的华北地区连续出现2次较强冷空气过程,造成大范围的低温、雨雪天气。利用北京地区11个气象站近50年逐日气温、降水资料,对全市历年11月低温雨雪事件的演变特征进行了分析。结果表明,2009年11月全市月平均气温、月平均最低气温均突破了50年的最低记录,月平均最高气温位列1981年11月之后,接近历史极值;2009年11月降雪量也位列有记录以来第一位,冰冻日数历史排位第三;从气温和降水极端事件发生的频次来看,2009年11月日平均气温、日最高气温和日最低气温通过5%分位值标准的极端低温事件频次都明显偏多,在50年中居于第2位,降水量通过95%分位值标准的极端强事件频次在50年中居于第四位。2009年11月的严重低温雨雪事件出现在区域气温总体变暖、低温事件频率总体下降的气候趋势背景下,在一定程度上放大了负面影响。亚洲中高纬地区500hPa高度场经向度异常加大、冷暖气流交换活跃,是造成2009年11月极端低温和大雪的直接环流因子。 相似文献
406.
A dataset of global ocean surface currents for 1999-2007 derived from Argo float trajectories: Comparison with surface drifter and TAO measurements
下载免费PDF全文
![点击此处可从《大气和海洋科学快报》网站下载免费的PDF全文](/ch/ext_images/free.gif)
A dataset of surface current vectors with error estimate from 1999 to 2007 is derived from the trajectories of the Array for Real-time Geostrophic Oceanography (Argo) drifting on surface over the global ocean. The error of the estimated surface currents is about 4.7 cm s-1 which is equivalent to the accuracy of the currents determined from the surface drifters. Geographically, the Argo-derived surface currents can fill many gaps left by the Global Drifter Program due to the greater number of floats, and can provide a complementary in situ observational system for monitoring global ocean surface currents. The surface currents from the Argo floats are compared with the surface drifter-derived currents and the Tropical Atmosphere Ocean program (TAO) measurements. The comparisons show good agreement for both the current amplitude and the direction of surface currents. Results indicate the feasibility of obtaining ocean surface currents from the Argo array and of combining the surface currents from Argo and the ocean surface drifters for in situ mapping of the global surface currents. The authors also make the dataset available to users of interest for many types of applications. 相似文献
407.
De-Fu Bu Feng Yuan Fu-Guo Xie 《Monthly notices of the Royal Astronomical Society》2009,392(1):325-331
Observations and numerical magnetohydrodynamic (MHD) simulations indicate the existence of outflows and ordered large-scale magnetic fields in the inner region of hot accretion flows. In this paper, we present the self-similar solutions for advection-dominated accretion flows (ADAFs) with outflows and ordered magnetic fields. Stimulated by numerical simulations, we assume that the magnetic field has a strong toroidal component and a vertical component in addition to a stochastic component. We obtain the self-similar solutions to the equations describing the magnetized ADAFs, taking into account the dynamical effects of the outflow. We compare the results with the canonical ADAFs and find that the dynamical properties of ADAFs such as radial velocity, angular velocity and temperature can be significantly changed in the presence of ordered magnetic fields and outflows. The stronger the magnetic field is, the lower the temperature of the accretion flow will be and the faster the flow rotates. The relevance to observations is briefly discussed. 相似文献
408.
Yi Xie Zhao-Yan Huang Xiang-Fu Jia Shao-Juan Fan Fang-Fang Liu 《Monthly notices of the Royal Astronomical Society》2009,398(2):583-590
We consider the influence of magnetic fields on the model of neutrino-dominated accretion flows (NDAFs) for gamma-ray bursts (GRBs) via the assumption that the accretion rate of the disc is totally caused by the torque of the Lorentz force, i.e. the magnetic braking of large-scale magnetic fields and magnetic viscosity of small-scale magnetic fields. We calculate the structure, composition, luminosity of neutrino emission and the Poynting flux, and the rate of mass loss driven by neutrino heating or launched centrifugally by large-scale magnetic fields, based on the physical condition of the magnetized NDAFs. It is shown that the magnetized disc is favourable to interpret the diverse prompt emissions as well as the X-ray flares observed in the early afterglow of GRBs. 相似文献
409.
In this paper, we present a study of the correlation between the speed of flare ribbon separation and the magnetic flux density
during the 10 April 2001 solar flare. The study includes the section of the neutral line containing the flare core and its
peripheral area. This event shows clear two-ribbon structure and inhomogeneous magnetic fields along the ribbons, so the spatial
correlation and distribution of the flare and magnetic parameters can be studied. A weak negative correlation is found between
the ribbon separation speed (V
r) and the longitudinal magnetic flux density (B
z
). This correlation is the weakest around the peak of the flare. Spatially, the correlation is also weakest at the positions
of the hard X-ray (HXR) sources. In addition, we estimate the magnetic reconnection rate (electric field strength in the reconnection
region E
rec) by combining the speed of flare ribbons and the longitudinal magnetic flux density. During flare evolution, the time profiles
of the magnetic reconnection rate are similar to that of the ribbon separation speed, and the speeds of ribbon separation
are relatively slow in the strong magnetic fields (i.e., V
r is negatively correlated with B
z
). However, along the flare ribbons, E
rec fluctuates in a small range except near the HXR source. A localized enhancement of the reconnection rate corresponds to the
position of the HXR source. 相似文献
410.
Gangjian Wei Malcolm T. McCulloch Graham Mortimer Luhua Xie 《Geochimica et cosmochimica acta》2009,73(8):2332-2346
Geochemical records preserved in the long-lived carbonate skeleton of corals provide one of the few means to reconstruct changes in seawater pH since the commencement of the industrial era. This information is important in not only determining the response of the surface oceans to ocean acidification from enhanced uptake of CO2, but also to better understand the effects of ocean acidification on carbonate secreting organisms such as corals, whose ability to calcify is highly pH dependent. Here we report an ∼200 year δ11B isotopic record, extracted from a long-lived Porites coral from the central Great Barrier Reef of Australia. This record covering the period from 1800 to 2004 was sampled at yearly increments from 1940 to the present and 5-year increments prior to 1940. The δ11B isotopic compositions reflect variations in seawater pH, and the δ13C changes in the carbon composition of surface water due to fossil fuel burning over this period. In addition complementary Ba/Ca, δ18O and Mg/Ca data was obtained providing proxies for terrestrial runoff, salinity and temperature changes over the past 200 years in this region. Positive thermal ionization mass spectrometry (PTIMS) method was utilized in order to enable the highest precision and most accurate measurements of δ11B values. The internal precision and reproducibility for δ11B of our measurements are better than ±0.2‰ (2σ), which translates to a precision of better than ±0.02 pH units. Our results indicate that the long-term pre-industrial variation of seawater pH in this region is partially related to the decadal-interdecadal variability of atmospheric and oceanic anomalies in the Pacific. In the periods around 1940 and 1998 there are also rapid oscillations in δ11B compositions equivalent changes in pH of almost 0.5 U. The 1998 oscillation is co-incident with a major coral bleaching event indicating the sensitivity of skeletal δ11B compositions to loss of zooxanthellate symbionts. Importantly, from the 1940s to the present-day, there is a general overall trend of ocean acidification with pH decreasing by about 0.2-0.3 U, the range being dependent on the value assumed for the fractionation factor α(B3-B4) of the boric acid and borate species in seawater. Correlations of δ11B with δ13C during this interval indicate that the increasing trend towards ocean acidification over the past 60 years in this region is the result of enhanced dissolution of CO2 in surface waters from the rapidly increasing levels of atmospheric CO2, mainly from fossil fuel burning. This suggests that the increased levels of anthropogenic CO2 in atmosphere has already caused a significant trend towards acidification in the oceans during the past decades. Observations of surprisingly large decreases in pH across important carbonate producing regions, such as the Great Barrier Reef of Australia, raise serious concerns about the impact of Greenhouse gas emissions on coral calcification. 相似文献