全文获取类型
收费全文 | 1501篇 |
免费 | 114篇 |
国内免费 | 107篇 |
专业分类
测绘学 | 134篇 |
大气科学 | 45篇 |
地球物理 | 305篇 |
地质学 | 256篇 |
海洋学 | 42篇 |
天文学 | 745篇 |
综合类 | 73篇 |
自然地理 | 122篇 |
出版年
2024年 | 6篇 |
2023年 | 6篇 |
2022年 | 16篇 |
2021年 | 17篇 |
2020年 | 15篇 |
2019年 | 24篇 |
2018年 | 15篇 |
2017年 | 31篇 |
2016年 | 30篇 |
2015年 | 30篇 |
2014年 | 33篇 |
2013年 | 64篇 |
2012年 | 30篇 |
2011年 | 36篇 |
2010年 | 45篇 |
2009年 | 84篇 |
2008年 | 93篇 |
2007年 | 157篇 |
2006年 | 93篇 |
2005年 | 78篇 |
2004年 | 85篇 |
2003年 | 77篇 |
2002年 | 92篇 |
2001年 | 59篇 |
2000年 | 76篇 |
1999年 | 57篇 |
1998年 | 55篇 |
1997年 | 79篇 |
1996年 | 38篇 |
1995年 | 39篇 |
1994年 | 35篇 |
1993年 | 26篇 |
1992年 | 20篇 |
1991年 | 12篇 |
1990年 | 15篇 |
1989年 | 10篇 |
1988年 | 18篇 |
1987年 | 15篇 |
1986年 | 5篇 |
1985年 | 3篇 |
1982年 | 2篇 |
1981年 | 1篇 |
排序方式: 共有1722条查询结果,搜索用时 15 毫秒
281.
利用UMRAO数据库22个耀变体源的偏振数据,根据Lazarian&Pogosyan理论模型分析研究了耀变体射电波段的偏振随波长的变化,得出不同类的耀变体偏振随波长变化的原因。结果表明,与Lazarian&Pogosyan理论模型吻合较好。由此得出如下结论:(1)反常去偏振耀变体源中反常法拉第旋光起主导作用,反常去偏振相对较少;(2)热辐射与同步辐射混合作用,高频波段的偏振度小于低频波段的偏振度(反常去偏振);(3)当被观测波段波长小于吸积盘热辐射对应的维恩波长时,高频波段的偏振度大于低频波段的偏振度(常规去偏振)。 相似文献
282.
283.
284.
285.
Andreas Burkert 《Astrophysics and Space Science》2003,284(2):697-700
The puzzling correlation between the spin parameter λ of galactic disks and the disk-to-halo mass fraction f
disk is investigated. It is shown that such a correlation arises naturally from large uncertainties in determining the virial
masses of dark matter halos. This result indicates that halo properties derived from fits to observed rotation curves are
still very uncertain. An analysis of λ versus f
disk as function of the adopted halo virial mass shows that for reasonable halo concentrations f
disk ≈ 0.01 - 0.07 which is significantly smaller than the universal baryon fraction. Most of the available gas either never settled
into the galactic disks or was ejected subsequently.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
286.
In this paper the tidal phenomena on the Earth are concisely specified, including solid tides, ocean tides and atmospheric tides due to the luni-solar tide-generating force, and the Earth pole tide due to the motion of the Earth's rotation axis (polar motion); as well as their effects on the Earth rotation. The outcomes of scientific researches of Chinese astronomers on these topics are described in some detail. These researches deal with the mechanisms responsible for tidal effects on the earth rotation, and on the measurements of the Earth rotation parameters. Finally, the effects discovered by Chinese researchers on the measurements of the period and change in period of pulsars are discussed. These effects are very small in magnitude but not negligible. 相似文献
287.
Jørgen Christensen-Dalsgaard 《Astrophysics and Space Science》2003,284(1):277-294
The workshop took place at the beginning of what promises tobe a golden age of asteroseismology.Ground-based instrumentation is finally reaching a level of stabilitywhich allows detailed investigations of solar-like oscillations in atleast bright, slowly rotating main-sequence stars.Very extensive results are expected from the coming space missions,including data on a broad range of stars from the Eddington mission.The observational situation is therefore extremely promising.To make full use of these promises, major efforts are requiredtowards the efficient utilization of the data, through the developmentof techniques for the analysis and interpretation of the data.A broad range of topics related to these issues is discussed in the presentproceedings. Here I review some of the relevant problems,relate the asteroseismic investigations to broader areas of astrophysics and consider briefly the basis for our great expectations for the developmentof the field. 相似文献
288.
We consider the effects of projection, internal absorption, and gas-or stellar-velocity dispersion on the measured rotation curves of galaxies with edge-on disks. Axisymmetric disk models clearly show that the rotational velocity in the inner galaxy is highly underestimated. As a result, an extended portion that imitates nearly rigid rotation appears. At galactocentric distances where the absorption is low (i.e., it does not exceed 0.3–0.5m kpc?1), the line profiles can have two peaks, and a rotation curve with minimum distortions can be obtained by estimating the position of the peak that corresponds to a higher rotational velocity. However, the high-velocity peak disappears in high-absorption regions and the actual shape of the rotation curve cannot be reproduced from line-of-sight velocity estimates. In general, the optical rotation curves for edge-on galaxies are of little use in reconstructing the mass distribution in the inner regions, particularly for galaxies with a steep velocity gradient in the central region. In this case, estimating the rotation velocities for outer (transparent) disk regions yields correct results. 相似文献
289.
大气对地球自转参数(ERP)的高频激发 总被引:4,自引:0,他引:4
本文采用1983—1992年期间由空间大地测量技术观测和归算的地球自转参数(ERP)序列,以及由全球气象资料归算的大气角动量(AAM)序列,分析和研究了大气对地球自转参数的日长变化(LOD)和极移(x和y)在一个月时间尺度以内的高频激发作用,得到的主要结果如下:1大气对LOD分量高频潮汐的估计值存在着影响,但是,潮汐形变参数k/c随时间和频率的变化却是受非大气因素的扰动引起的.2.大气可以解释30天以下LOD非潮汐的大部分变化.3.极移分量30天以内的高频变化也主要由大气激发.x分量与大气的相关性要强于y分量,而且更为稳定,主要表现为平均时间尺度约为27天的波动,大气对这个波动的贡献可达70%. 相似文献
290.