全文获取类型
收费全文 | 7901篇 |
免费 | 1012篇 |
国内免费 | 1645篇 |
专业分类
测绘学 | 718篇 |
大气科学 | 2182篇 |
地球物理 | 1468篇 |
地质学 | 4318篇 |
海洋学 | 683篇 |
天文学 | 323篇 |
综合类 | 277篇 |
自然地理 | 589篇 |
出版年
2024年 | 30篇 |
2023年 | 116篇 |
2022年 | 111篇 |
2021年 | 120篇 |
2020年 | 37篇 |
2019年 | 107篇 |
2018年 | 150篇 |
2017年 | 133篇 |
2016年 | 193篇 |
2015年 | 142篇 |
2014年 | 726篇 |
2013年 | 315篇 |
2012年 | 183篇 |
2011年 | 288篇 |
2010年 | 156篇 |
2009年 | 110篇 |
2008年 | 217篇 |
2007年 | 150篇 |
2006年 | 134篇 |
2005年 | 156篇 |
2004年 | 120篇 |
2003年 | 276篇 |
2002年 | 1804篇 |
2001年 | 1947篇 |
2000年 | 480篇 |
1999年 | 137篇 |
1998年 | 118篇 |
1997年 | 103篇 |
1996年 | 130篇 |
1995年 | 170篇 |
1994年 | 139篇 |
1993年 | 148篇 |
1992年 | 200篇 |
1991年 | 178篇 |
1990年 | 230篇 |
1989年 | 150篇 |
1988年 | 125篇 |
1987年 | 80篇 |
1986年 | 54篇 |
1985年 | 77篇 |
1984年 | 50篇 |
1983年 | 51篇 |
1982年 | 40篇 |
1981年 | 29篇 |
1980年 | 55篇 |
1979年 | 13篇 |
1978年 | 16篇 |
1977年 | 9篇 |
1976年 | 6篇 |
1964年 | 5篇 |
排序方式: 共有10000条查询结果,搜索用时 218 毫秒
21.
Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field. 相似文献
22.
高频VLBI观测揭示出河外射电源在pc或者亚pc尺度上大都有核-喷流的内部结构,尤其是对平谱致密射电源中毫角秒尺度的子源,能以相当高的概率观测到它的视超光速现象。多频观测可监测到一些新喷流子源的出现,特别在射电激变源中这些新喷流子源的出现与宽带内(从光学到γ射线)的爆发相关。且得到的一些源的核区谱指数分布,为确认源的VLBI核提供了支持。 相似文献
23.
引言 D.布鲁金尼的论文《可用空间时代技术进行更精确的人口普查》提出了一些有趣的问题。我们为能够在《摄影测量工程和遥感》杂志上看到这篇有关遥感在社会科学领城内的应用的论文而高兴。我们认为只有了解人口普查数据的多种用途之后,再来检验那些改进人口普查的方法才是合适的,众所周知,每十年一次的人口普查数据的精度和完备性并不是没有缺点的。无疑地,许多人口普查人员将首先承认,每次由点数 相似文献
24.
奶牛隐性乳房炎发生规律探讨 总被引:4,自引:0,他引:4
通过对某奶牛场泌乳牛群隐性乳房炎的调查和分析。研究了奶牛隐性乳房炎的发生规律。结果表明,该场奶牛隐性乳房炎的阳性率为31.42%。乳区临诊阳性率达到10.60%。隐性乳房炎的发生随着胎次和泌乳时间的增加而增加,左乳区阳性率高于右侧,前乳区高于后乳区,在牛群(场)里进行经常性的临床和实验室检验是必要的。 相似文献
25.
The δ Scuti star ctalogue is used to derive the observational locations of such stars on the HR diagram.The theoretical and observational instability strips are compared to check the theoretical red edge obtained by considering nonlocal time-dependent convection theory.The observational instability strip almost overlaps with the theoretical one,but the observed blue and red envelopes are hotter overlaps with the theoretical one,but the observed blue and red envelopes are hotter than the theoretical edges.The distribution of δ Scuti stars in the pulsation strip is not uniform. 相似文献
26.
对天区0112-35的UKST物端棱镜底片上的11个类星体候选者进行了光谱观测,证实为类星体,给出了它们的红移值、证认图及光谱图。11个类星体中有6个属于角距小于4角分的3对类星体;1个类星体-星系对。 相似文献
27.
28.
作者用透射电子显微镜研究了沉积钙质白云石中的带状面缺陷。在衍衬象中面缺陷呈现出特有的条纹衬度,并具有一定的择优取向,它们沿着{018}面排列。面缺陷也可分叉,分枝部分平等于{2-/10}面。根据白云石面缺陷的取向,本文提出了鞍状白云石宏观弯曲面和微观面缺陷的取向关系。 相似文献
29.
We have obtained velocity-resolved spectra of the 12C II 157.8 microns 2P3/2-2P1/2 fine structure line in the M42 region of Orion. Observations at 0.8 km s-1 resolution with a laser heterodyne spectrometer show multiple velocity components in some locations, with typical linewidths of 3-5 km s-1. Spectra of theta 1C and BN-KL also show weak emission from the F = 2-1 hyperfine component of the equivalent 13C II line. From the observed 12C II/13C II line intensity ratios, we deduce that the 12C II emission is optically thick with tau approximately 5 at both positions. Excitation temperatures of 128 K and 90 K, together with column densities of approximately 1 x 10(19) cm-2 and approximately 4 x 10(18) cm-2, are derived for theta 1C and BN-KL, respectively. 相似文献
30.
We have used observations of the rare isotopes of HCN and HNC to determine the relative abundance of these two chemical isomers along the central ridge of the Orion molecular cloud. The abundance ratio [HCN]/[HNC] decreases by more than an order of magnitude from the relatively warm plateau and hot core sources toward the KL nebula to the colder, more quiescent clouds to the north and south. Even in the cooler regions, however, the ratio is an order of magnitude larger than that found in previous investigations of cold dark clouds. We determine the kinetic temperature in the regions we have studied from new observations of methylacetylene (CH3CCH), together with other recent estimates of the gas temperature near KL. The results suggest that the warmer portions of the cloud are dominated by different chemical pathways than those in the general interstellar cloud material. 相似文献