全文获取类型
收费全文 | 1254篇 |
免费 | 141篇 |
国内免费 | 125篇 |
专业分类
测绘学 | 374篇 |
大气科学 | 76篇 |
地球物理 | 246篇 |
地质学 | 287篇 |
海洋学 | 91篇 |
天文学 | 133篇 |
综合类 | 117篇 |
自然地理 | 196篇 |
出版年
2023年 | 7篇 |
2022年 | 31篇 |
2021年 | 48篇 |
2020年 | 47篇 |
2019年 | 56篇 |
2018年 | 40篇 |
2017年 | 70篇 |
2016年 | 59篇 |
2015年 | 63篇 |
2014年 | 65篇 |
2013年 | 84篇 |
2012年 | 70篇 |
2011年 | 81篇 |
2010年 | 62篇 |
2009年 | 86篇 |
2008年 | 76篇 |
2007年 | 98篇 |
2006年 | 65篇 |
2005年 | 57篇 |
2004年 | 45篇 |
2003年 | 45篇 |
2002年 | 42篇 |
2001年 | 27篇 |
2000年 | 32篇 |
1999年 | 32篇 |
1998年 | 20篇 |
1997年 | 15篇 |
1996年 | 14篇 |
1995年 | 16篇 |
1994年 | 9篇 |
1993年 | 6篇 |
1992年 | 9篇 |
1991年 | 8篇 |
1990年 | 2篇 |
1989年 | 11篇 |
1988年 | 7篇 |
1987年 | 6篇 |
1986年 | 2篇 |
1985年 | 3篇 |
1982年 | 1篇 |
1980年 | 2篇 |
1971年 | 1篇 |
排序方式: 共有1520条查询结果,搜索用时 15 毫秒
881.
Ujsing deterministic methods in combination with probabilistic methods,the authors havestudied in detail the seismogeological background,seismogfnic faults and their abilities ingenerating earthquakes,the temporal and spatial distribution features of seismicity;predicted the seismicity tendency in future 50 years;and studied the expected magnitude andexpected distance of destructive earthquakes that may attack Zigong City.On such a basis,2scenario earthquakes have been determined for Zigong City.The results would be helphl forthe lecal government and authorities to work out a great earthquake emergency pre-plan andto estaplish the great earthquake fast-response system. 相似文献
882.
Low velocity zone of upper mantle and its effect on PdSwr phase related to 670 km discontinuity 总被引:2,自引:2,他引:0
This paper studied some properties of PdSwr phase related to 670 km discontinuities in detail, and theoretically processed a preliminary analysis to this phase. We discussed the relationships between the incident angle ih of PdSwr phase with its path, epicentral distance, travel-time and relative amplitude due to low velocity zone (LVZ) of upper mantle, and preliminarily pointed out the main characters of PdSwr phase recorded in seismogram. The PdSwr phase is concentrated in range of 13.5(~96.5(. When epicentral distance is greater than 33(, the start point of PdSwr phase is relatively well distinguishable and could thus be determined more easily. When the epicentral distance is between 13.5( to 33(, the triplication of PdSwr(s travel-time curve could be slightly distinguished due to the low velocity zone and 220 km seismic velocity discontinuity of upper mantle. The relevant observed PdSwr phase should be in a more complex pattern and it should be more difficult to determine its start point. 相似文献
883.
W. P. S. Meikle 《Monthly notices of the Royal Astronomical Society》2000,314(4):782-792
The absolute luminosities and homogeneity of early-time infrared (IR) light curves of type Ia supernovae are examined. Eight supernovae are considered. These are selected to have accurately known epochs of maximum blue light as well as having reliable distance estimates and/or good light curve coverage. Two approaches to extinction correction are considered. Owing to the low extinction in the IR, the differences in the corrections via the two methods are small. Absolute magnitude light curves in the J , H and K bands are derived. Six of the events, including five established 'branch-normal' supernovae, show similar coeval magnitudes. Two of these, supernovae (SNe) 1989B and 1998bu, were observed near maximum infrared light. This occurs about 5 d before maximum blue light. Absolute peak magnitudes of about −19.0, −18.7 and −18.8 in J , H and K respectively were obtained. The two spectroscopically peculiar supernovae in the sample, SNe 1986G and 1991T, also show atypical IR behaviour. The light curves of the six similar supernovae can be represented fairly consistently with a single light curve in each of the three bands. In all three IR bands the dispersion in absolute magnitude is about 0.15 mag, and this can be accounted for within the uncertainties of the individual light curves. No significant variation of absolute IR magnitude with B -band light curve decline rate, Δ m 15 ( B ), is seen over the range 0.87<Δ m 15 ( B )<1.31. However, the data are insufficient to allow us to decide whether or not the decline rate relation is weaker in the IR than in the optical region. IR light curves of type Ia supernovae should eventually provide cosmological distance estimates that are of equal, or even superior, quality to those obtained in optical studies. 相似文献
884.
The Nearby Supernova Factory is an international project dedicated to the study of the nearby thermonuclear (type Ia) supernovæ. Based upon the NEAT search for the target discovery and the dedicated integral field spectrograph SNIFS for the follow‐up, the goal is to study, over a continuous period of 4 years, the spectro‐photometric evolution of ∼300 SNe Ia at z < 0.08 from −15 to +50 days in the extended optical range (320–1000 nm). This will allow to probe in detail the local Hubble diagram, SNe Ia physics and the SNe‐host galaxy correlations, serving as an unprecedented nearby benchmark for the high‐z cosmological studies to come. (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
885.
节织纹螺(Nassarius hepaticus)贝壳差异的COⅠ基因分析 总被引:1,自引:0,他引:1
选择在厦门港市场购买的节织纹螺(Nassarius hepaticus),挑选五种典型贝壳形态,每种形态各5个个体,研究其COⅠ基因序列及其分子系统发育。结果表明,节织纹螺五种贝壳类型的齿舌形态基本一致,但个体间齿列数和中央齿上缘小齿数有差异;COⅠ基因序列存在较大的变异,678—679bp的片段上有31个变异位点,其中20个为密码子第三位碱基,6个为密码子第二位碱基,5个为密码子第一位碱基;贝壳、齿舌变异与DNA变异不存在关系,同类型和不同类型的个体在DNA序列上差异较小,根据Kimura 2-parameter法计算25个个体的遗传距离在0.001—0.010之间,平均值为0.007。以COⅠ基因序列计算的遗传距离和构建的系统发育树证实五种贝壳形态的25个个体同属于节织纹螺。 相似文献
886.
通过形状匹配技术以获取等高线之间的相似程度,通过构建等高线树以获得等高线之间的邻近程度,然后将邻近的且形态相似的等高线实施聚类,实验结果表明聚类结果正确可靠。在获得聚类结果的基础上,还对等高线图进行了地形特征提取和数据压缩。 相似文献
887.
888.
889.
给出了星地双向上下行伪距观测的数学模型。利用Compass-M1卫星2007-11-25~2007-11-30的实测数据进行了钟差计算,并利用计算结果分别采用3种方案进行了短期、长期钟差预报。总结了钟差预报精度随拟合时间的变化规律,分析了其产生的原因,并给出了有益的结论。 相似文献
890.
Identifying barriers of species and characterize their effects on spatial distribution provide essential information to research
in landscape genetics. We propose a weighted difference barrier (WDB) method as an alternative to maximum difference barriers
(MDB), and to initiate and integrate more spatial modeling and methods into the problem solving process. Overall, WDB provides
quick and straightforward improvements to the drawbacks of MDB. WDB integrates more sample location relationships into the
barrier construction and reveals potential barriers that would otherwise go undetected. WDB incorporates both within group
and between group genetic information, and delineates the barriers as a more complex pattern.
相似文献
John RadkeEmail: |