全文获取类型
收费全文 | 1107篇 |
免费 | 176篇 |
国内免费 | 261篇 |
专业分类
测绘学 | 105篇 |
大气科学 | 228篇 |
地球物理 | 228篇 |
地质学 | 519篇 |
海洋学 | 147篇 |
天文学 | 77篇 |
综合类 | 127篇 |
自然地理 | 113篇 |
出版年
2024年 | 9篇 |
2023年 | 21篇 |
2022年 | 35篇 |
2021年 | 48篇 |
2020年 | 32篇 |
2019年 | 43篇 |
2018年 | 56篇 |
2017年 | 49篇 |
2016年 | 44篇 |
2015年 | 58篇 |
2014年 | 66篇 |
2013年 | 57篇 |
2012年 | 46篇 |
2011年 | 68篇 |
2010年 | 58篇 |
2009年 | 55篇 |
2008年 | 45篇 |
2007年 | 45篇 |
2006年 | 47篇 |
2005年 | 37篇 |
2004年 | 43篇 |
2003年 | 45篇 |
2002年 | 68篇 |
2001年 | 88篇 |
2000年 | 49篇 |
1999年 | 55篇 |
1998年 | 36篇 |
1997年 | 32篇 |
1996年 | 35篇 |
1995年 | 34篇 |
1994年 | 36篇 |
1993年 | 22篇 |
1992年 | 17篇 |
1991年 | 13篇 |
1990年 | 18篇 |
1989年 | 7篇 |
1988年 | 8篇 |
1987年 | 10篇 |
1985年 | 4篇 |
1984年 | 1篇 |
1983年 | 2篇 |
1982年 | 1篇 |
1964年 | 1篇 |
排序方式: 共有1544条查询结果,搜索用时 15 毫秒
171.
C. -H. You D. -I. Lee S. -M. Jang M. Jang H. Uyeda T. Shinoda F. Kobayashi 《Asia-Pacific Journal of Atmospheric Sciences》2010,46(1):41-51
The rainy season from June to July in the East Asia is called the Changma in Korea, the Meiyu in China, or the Baiu in Japan. The mesoscale convective systems which occur near a front frequently lead to severe weather phenomenon such as localized gust and heavy rainfall. An intensive field experiment was conducted at Chujado (33.95°N, 126.28°E) to find out the characteristics of the precipitating system using information such as the raindrop size distribution, kinematic features during a Changma period between June 21 2007 and July 11 2007. Different characteristics of three identified rainfall cases in a Changma frontal precipitation system occurred from 5 to 6 July in 2007 at Chujado area have been identified. Based on the radar reflectivity and raingage at Chujado, each rainfall system maintained for 7 hours, 4 hours, and 9 hours, respectively. According to the analysis of a total vertical wind shear (TVWS) and a directional vertical wind shear (DVWS), the temperature gradient was the strongest near the surface and both warm and cold advections were occurred in all cases but at different levels. The deep warm advection was related to the longer rainfall lifetime and stronger rainrate, but smaller raindrop size. The unstable atmospheric condition, which has cold advection at the surface and warm advection in higher level, caused the larger size diameter of raindrop. The echo top height of 30 dBZ was around 6 km in the two rainfall systems and around 4 km in the other one. The number concentrations of raindrop has turning point at the drop size of 2 mm in diameter. The stronger (weaker) updraft and downdraft were also related to the decreased number concentration of smaller (larger) size drops and increased that of the larger (smaller) drops. 相似文献
172.
利用中国科学院青藏高原研究所纳木错多圈层综合观测研究站在念青唐古拉峰扎当冰川垭口(30.47°N、90.65°E,5800m)和纳木错站(30.77°N、90.99°E,4730m)的逐日平均气温、相对湿度、气压等资料,与同期NCEP/NCAR再分析资料进行了对比分析,讨论了再分析资料在纳木错流域湖泊/冰川区气候变化研究中的适用性.结果表明:扎当冰川垭口和纳木错站气压再分析资料的可信度好于气温,相对湿度稍差:扎当冰川垭口气压和相对湿度再分析值与实测值的差值在冬季偏大,夏季偏小,气温则相反.在研究期间,总体上再分析资料在冰川区的可信度好于湖泊区,再分析资料能很好地反映该地区地面气压、气温和相对湿度的日变化特征,在应用到该地区气候变化的研究时应考虑地形的影响. 相似文献
173.
174.
175.
On 11 January 2002, using the Multi-channel Infrared Solar Spectrograph (MISS) at the Purple Mountain Observatory (PMO), we obtained Hα, Ca ii 8542 Å and He i 10?830 Å spectra and slit-jaw Hα images of a peculiar solar limb event. A close resemblance of its intensity to that of a small flare and the GOES X-ray flux indicates that it was an active prominence. However, its morphological evolution and velocity variation were different from general typical active prominences, such as limb flares, post-flare loops, surges and sprays. It started with the ejection of material from the flare site. In the early phase, the ejecta was as bright as a limb flare and kept rising until reaching the height of (8????10)×104 km at an almost constant velocity of 91.7 km? s ?1 with its lower part always connected to the solar surface. EUV images in 195 Å show similar structure as in the Hα line, indicating the coexistence of plasmas with temperatures differing by more than two orders of magnitude. Later some material started to fall back to another bright area on the solar surface. The falling material did not show the collimated structure of surges or the arc structure of flaring arches. A red-shift velocity of more than 200 km? s ?1 was detected in a bright point close to the outer edge of the closed loop system formed later, which dispersed in a few minutes and became a part of the newly formed large loop. The ejected material did not leave the sun, indicating that the magnetic reconnection was not sufficient to remove the overlying field lines during the process. The spectral line profiles showed large widths and variable velocities, and therefore the line-pair method is not applicable to this event for the estimation of physical parameters. 相似文献
176.
对太平洋500hPa候高度场和距平场进行了主成分分析,得出反映500hPa候高度特征的典型场。指出候高度场的第1特征向量的空间型是季节变化的主要型,它可解释总方差的74.5%,候高度场的其余特征向量与距平场的特征向量是按顺序的对应相似。这些典型场可以很好地描述北太平洋的大气环流特征。距平场的第1特征向量空间型清楚地反映了与厄尔·尼诺现象有关的环流型。 相似文献
177.
随着经济发展,人类经济社会对资源与能源的需求日益增加.我国在采资源正在枯竭,供需矛盾不断加大,对外依存度较高.国家对陆地盲区、深地和深海的资源勘探极为重视,同时未来勘探对象更为隐蔽、地质条件更为复杂,勘探与开采难度越来越大.地球物理方法作为勘查技术中最有效准确的预测方法之一,为满足勘探任务的需求,近年来地球物理勘探在研究新技术、新方法、仪器研发和数据处理解释等方面取得突破性进展.本文详细阐述我国的金属矿、煤矿、油气以及非常规油气资源的勘探开发现状,归纳了相应领域的地球物理技术新进展,对深地资源的勘探开发进行了展望,为资源与能源开发提供参考. 相似文献
178.
179.
We have pointed out that, when thermal relativistic electrons with an isotropic velocity distribution move through a region of dense gas or impinge upon its surface, the Cerenkov effect will produce a particular kind of atomic or ionic emission line, which we have called the “Cerenkov line-like radiation”. This prediction for the optical wavebands has been verified by laboratory experiments. In this paper, we extend this line-like radiation theory to the X-ray waveband and give the basic formulae for calculating the intensity ratio and intrinsic redshift ratio of the Cerenkov iron Kα and Kβ lines, for different ionization orders of iron. Potential application of this calculated result may be found in the study of AGNs. The recent observations of NGC3783 show that besides the iron Kα line at ∼6.4 keV, there is also a very strong iron Kβ line at ∼7.0 keV, and that the ratio of equivalent widths between the two is anomalous: EWKα/EWKβ ≈ 3.43. It is difficult to explain this by the conventional mechanism of “photoelectric absorption-fluorescence emission”. We suggest that the mechanism of Cerenkov line-like radiation can provides a way of solving this puzzle. Besides, we expect that the calculated intrinsic redshift ratio of Cerenkov iron Kα and Kβ lines could be tested in future observations. If our suggestion is further supported by observations, then our view on the physical environment around the central massive black hole of an AGN will be greatly modified: the activity becomes more energetic and violent, and the gas, much denser than previously thought. 相似文献
180.
东营凹陷下第三系层序地层研究与隐蔽油气藏预测 总被引:18,自引:3,他引:15
应用层序地层学理论,利用地震、测井、岩心和分析化验资料,建立了东营凹陷下第三系层序界面识别标志,把东营凹陷下第三系划分为 1个超层序组,4个超层序,10个层序,进行体系域划分,建立了东营凹陷下第三系层序地层格架。构造坡折带是指由同沉积构造长期活动引起的沉积斜坡明显突变的地带,对盆地充填的可容纳空间和沉积作用可产生重要影响。通过层序地层格架与构造坡折带的研究,建立东营凹陷层序发育模式。受构造坡折带控制的层序低位域砂体和湖侵体系域砂体,成藏条件良好,最有利于形成隐蔽油气藏。 相似文献