全文获取类型
收费全文 | 13444篇 |
免费 | 3001篇 |
国内免费 | 1390篇 |
专业分类
测绘学 | 90篇 |
大气科学 | 612篇 |
地球物理 | 9292篇 |
地质学 | 3981篇 |
海洋学 | 1074篇 |
天文学 | 594篇 |
综合类 | 746篇 |
自然地理 | 1446篇 |
出版年
2024年 | 27篇 |
2023年 | 122篇 |
2022年 | 328篇 |
2021年 | 422篇 |
2020年 | 473篇 |
2019年 | 559篇 |
2018年 | 468篇 |
2017年 | 446篇 |
2016年 | 396篇 |
2015年 | 482篇 |
2014年 | 645篇 |
2013年 | 669篇 |
2012年 | 730篇 |
2011年 | 754篇 |
2010年 | 687篇 |
2009年 | 849篇 |
2008年 | 798篇 |
2007年 | 979篇 |
2006年 | 950篇 |
2005年 | 808篇 |
2004年 | 838篇 |
2003年 | 718篇 |
2002年 | 610篇 |
2001年 | 458篇 |
2000年 | 546篇 |
1999年 | 454篇 |
1998年 | 433篇 |
1997年 | 360篇 |
1996年 | 381篇 |
1995年 | 304篇 |
1994年 | 282篇 |
1993年 | 230篇 |
1992年 | 168篇 |
1991年 | 107篇 |
1990年 | 75篇 |
1989年 | 77篇 |
1988年 | 54篇 |
1987年 | 45篇 |
1986年 | 33篇 |
1985年 | 16篇 |
1984年 | 5篇 |
1983年 | 3篇 |
1982年 | 6篇 |
1981年 | 6篇 |
1980年 | 2篇 |
1979年 | 20篇 |
1978年 | 2篇 |
1954年 | 10篇 |
排序方式: 共有10000条查询结果,搜索用时 0 毫秒
11.
Hong-Qi Zhang Xing-Ming Bao Yin Zhang Ji-Hong Liu Shu-Dong Bao Yuan-Yong Deng Wei Li Jie Chen Jin-Ping Dun Jiang-Tao Su Juan Guo Xiao-Fan Wang Ke-Liang Hu Gang-Hua Lin Dong-Guang WangNational Astronomical Observatories Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2003,3(6):491-494
We analyze the magnetic configurations of three super active regions, NOAA 10484, 10486 and 10488, observed by the Huairou Multi-Channel Solar Telescope (MCST) from 2003 October 18 to November 4. Many energetic phenomena, such as flares (including a X-28 flare) and coronal mass ejections (CMEs), occurred during this period. We think that strong shear and fast emergence of magnetic flux are the main causes of these events. The question is also of great interest why these dramatic eruptions occurred so close together in the descending phase of the solar cycle. 相似文献
12.
应用GPS观测青藏高原东北缘应力场变化 总被引:2,自引:0,他引:2
采用各向同性弹性地球模型推导了地面位移场速率与地壳内任意点应力场变化的边界积分关系,同时利用青藏高原东北缘1999~2001年观测的GPS资料对观测区地壳深度为5 km和25 km的主应力和最大剪应力进行了计算分析.结果表明,青藏高原东北缘的主应力变化主要集中在祁连山断裂、海原断裂等,在1920~1954年间历史上发生过多次震级为7.0~8.5级强震的断裂附近,并具有主应力变化沿断层走向分布、最大剪应力沿断层走向交替变化等特征. 相似文献
13.
Synthetic SH seismograms in a laterally varying medium by the discrete wavenumber method 总被引:1,自引:0,他引:1
Summary. We present a new method to calculate the SH wavefield produced by a seismic source in a half-space with an irregular buried interface. The diffracting interface is represented by a distribution of body forces. The Green's functions needed to solve the boundary conditions are evaluated using the discrete wavenumber method. Our approach relies on the introduction of a periodicity in the source-medium configuration and on the discretization of the interface at regular spacing. The technique developed is applicable to boundaries of arbitrary shapes and is valid at all frequencies. Some examples of calculation in simple configurations are presented showing the capabilities of the method. 相似文献
14.
中国大陆科学钻探先导孔零偏VSP资料解释 总被引:3,自引:3,他引:0
用六级三分量检波器在中国大陆科学钻探先导孔中实施了零偏VSP测量.数据处理结果表明,中国大陆科学钻探孔区超高压变质岩石的地震波速度主要介于4500~7000m/s之间,显著高于一般的沉积岩地区,而且随深度变化不明显.声波测井速度系统地稍低于VSP层速度,可能是由于井壁处岩石的完整性受到破坏而造成的.地震波速度与岩石密度和岩性存在明确的对应关系,榴辉岩的密度和地震波速度均显著高于片麻岩类岩石;由榴辉岩退变生成的斜长角闪岩类岩石,其密度和地震波速度均呈现出较大的变化,主要与其退变质程度有关;超基性岩中的裂隙系统导致其密度和地震波速度大幅度下降.由于榴辉岩与其他岩石类型之间存在较大的波阻抗差异,因此用零偏VSP资料标定该区地震波的地质层位是有效的.关于地震波反射的原因,通过综合研究地震波(包括反射纵波、上行转换横波、井筒波)的特征、岩石速度和密度分布以及井径变化,认为主要是岩性分界面、韧性剪切带和断裂(带),但还有一些因素尚待进一步研究. 相似文献
15.
16.
C. Debi Prasad Ashok Ambastha Nandita Srivastava Sushanta C. Tripathy Mona J. Hagyard 《Journal of Astrophysics and Astronomy》1997,18(1):39-55
Super-active region NOAA 6555 was highly flare productive during the period March 21st–27th, 1991 of its disk passage. We
have st udied its chromospheric activity using high spatial resolution Hα filtergrams taken at Udaipur along with MSFC vector
magnetograms. A possible relationship of flare productivity and the variation in shear has been explored. Flares were generally
seen in those subareas of the active region which possessed closed magnetic field configuration, whereas only minor flares
and/or surges occurred in subareas showing open magnetic field configuration. Physical mechanisms responsible for the observed
surges are also discussed. 相似文献
17.
Surface waters of Alsea Bay, an unpolluted estuary on the Oregon coast, were analysed for nitrous oxide, nitrate and nitrite on a weekly or biweekly basis during the summer of 1979. The estuary was found to be a variable source of N2O to the atmosphere. Large and rapid increases in the concentrations of N2O, NO3?, and NO2? occurred at the beginning of the sampling period and are attributed to the influx of nutrient-rich upwelling water into the estuary with the tide. The subsequent decline in concentrations of nitrate, nitrite and nitrous oxide over the remainder of the summer is attributed to a decrease in upwelling intensity, a decline in nitrification rates and to assimilatory nitrate reduction. Measurements of nitrous oxide at six stations along the Alsea River were also made in September and October before and after the onset of the rainy season. Samples taken after flood conditions were established were systematically 50% higher than pre-flood samples. The data suggest that soil runoff results in elevated concentrations of N2O in rivers. 相似文献
18.
本文对第22太阳周(1987年1月至1992年12月)中发生过M级以上的X射线耀斑(Hα耀斑级别≥M级,并伴有X射线的耀斑)对应的395个活动区资料进行了耀斑指数的统计,得到的结果:1.22太阳周M级以上X射线耀斑级别综合指数表,2.22太阳周M级以上X射线耀斑总指数表,3.第22太阳周M级以上X射线耀斑总指数随时间的变化曲线,4.第22太阳周M级以上X射线濯斑总指数直方图,该图表明第22太阳周活动的极大年分别是1989和1991年,为第23周太阳活动预报提供了可用参数。 相似文献
19.
20.
We present radio interferometric observations of the Algol-type binary system RZ Cassiopeiae made with the VLA and MERLIN arrays at 6 cm over an incomplete orbital cycle of the system (1.195 d). We detected RZ Cas with both instruments. The images were unresolved in both cases, with angular extents comparable to the synthesized beams. The peak flux density in the VLA image was 1.14 mJy beam−1 and in the MERLIN image it was 0.93 mJy beam−1 . The derived brightness temperatures are 4.02 × 108 and 4.35 × 108 K and the effective electron energies are 0.347 and 0.346 MeV for the MERLIN and VLA data respectively. The radio light curve shows an interesting modulation centred close to the primary eclipse which seems to correlate with ASCA SIS observations of the system. The results can be interpreted as an emitting region on the outer hemisphere of the cool component aligned along the centroid axis of the binary system. 相似文献