全文获取类型
收费全文 | 23062篇 |
免费 | 4348篇 |
国内免费 | 5900篇 |
专业分类
测绘学 | 322篇 |
大气科学 | 629篇 |
地球物理 | 2014篇 |
地质学 | 20577篇 |
海洋学 | 1729篇 |
天文学 | 5137篇 |
综合类 | 964篇 |
自然地理 | 1938篇 |
出版年
2024年 | 84篇 |
2023年 | 366篇 |
2022年 | 795篇 |
2021年 | 937篇 |
2020年 | 918篇 |
2019年 | 1163篇 |
2018年 | 1044篇 |
2017年 | 1184篇 |
2016年 | 1312篇 |
2015年 | 1180篇 |
2014年 | 1546篇 |
2013年 | 1601篇 |
2012年 | 1586篇 |
2011年 | 1747篇 |
2010年 | 1593篇 |
2009年 | 2015篇 |
2008年 | 1827篇 |
2007年 | 1836篇 |
2006年 | 1592篇 |
2005年 | 1386篇 |
2004年 | 1159篇 |
2003年 | 1011篇 |
2002年 | 847篇 |
2001年 | 718篇 |
2000年 | 655篇 |
1999年 | 647篇 |
1998年 | 427篇 |
1997年 | 356篇 |
1996年 | 299篇 |
1995年 | 267篇 |
1994年 | 251篇 |
1993年 | 213篇 |
1992年 | 171篇 |
1991年 | 123篇 |
1990年 | 97篇 |
1989年 | 70篇 |
1988年 | 59篇 |
1987年 | 26篇 |
1986年 | 28篇 |
1985年 | 32篇 |
1984年 | 28篇 |
1983年 | 25篇 |
1982年 | 21篇 |
1981年 | 12篇 |
1980年 | 20篇 |
1979年 | 7篇 |
1978年 | 5篇 |
1977年 | 16篇 |
1954年 | 2篇 |
1875年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 31 毫秒
151.
152.
153.
154.
We present a 2D general circulation model of Titan's atmosphere, coupling axisymmetric dynamics with haze microphysics, a simplified photochemistry and eddy mixing. We develop a parameterization of latitudinal eddy mixing by barotropic waves based on a shallow-water, longitude-latitude model. The parameterization acts locally and in real time both on passive tracers and momentum. The mixing coefficient varies exponentially with a measure of the barotropic instability of the mean zonal flow. The coupled GCM approximately reproduces the Voyager temperature measurements and the latitudinal contrasts in the distributions of HCN and C2H2, as well as the main features of the zonal wind retrieved from the 1989 stellar occultation. Wind velocities are consistent with the observed reversal time of the North-South albedo asymmetry of 5 terrestrial years. Model results support the hypothesis of a non-uniform distribution of infrared opacity as the cause of the Voyager temperature asymmetry. Transport by the mean meridional circulation, combined with polar vortex isolation may be at the origin of the latitudinal contrasts of trace species, with eddy mixing remaining restricted to low latitudes most of the Titan year. We interpret the contrasts as a signature of non-axisymmetric motions. 相似文献
155.
广西中三叠统浊流流向及坡向 总被引:1,自引:0,他引:1
通过对广西中三叠统浊积岩系中溢堤流沉积的识别,结合同一鲍马层序Tc段斜层理倾向与其底部槽模走向不一致的分析,以及横向冲刷模、U形障碍冲刷痕等冲蚀构造、大型滑动模等压刻构造的认识,筛选出宽阔水道充填沉积、扇状体及分支水道沉积中底模构造的指向数据,来指示浊流主体流向,并区分出溢堤流流向。从而确定了本区中三叠世时的浊流主体流向为NW向,平均为300°。根据滑塌沉积中滑塌包卷层轴面、滑塌面的测定,确定凤山县金牙处的古坡向平均为322°,与浊流主体流向基本一致。还认为中三叠世时右江盆地沉积物源来自桂东和桂东南蚀源区,海水由其南的越南境内进入。 相似文献
156.
辽宁东、西部地质上诸多差异并非是原地升降运动造成的,而是二个异地岩块经郯庐断裂大规模左旋平移运动迁移到一起的结果。辽东半岛原曾与鲁西-徐淮地区处于相同的古纬度。郯庐断裂北延的主干断裂应是抚顺-敦化断裂,它在辽宁境内是地层区划的重要界线。郯庐断裂在太古宙末期即已出现,曾多次变换其平移方向,最近一次大规模左行平移活动的高峰期是在晚侏罗世晚期-早白垩世,结束于孙家湾组或泉头组堆积之前。 相似文献
157.
J. P. Bernstein † Suketu P. Bhavsar ‡ 《Monthly notices of the Royal Astronomical Society》2001,322(3):625-630
The brightest, or first-ranked, galaxies (BCGs) in rich clusters show a very small dispersion in luminosity, making them excellent standard candles. This small dispersion raises questions about the nature of BCGs. Are they simply the extremes of normal galaxies formed via a stochastic process, or do they belong to a special class of atypical objects? If they do, are all BCGs special, or do normal galaxies compete for the first rank? To answer these questions, we undertake a statistical study of BCG magnitudes using results from extreme value theory. Two-population models do better than one-population models. A simple scenario where a random boost in the magnitude of a fraction of bright normal galaxies forms a class of atypical galaxies best describes the observed distribution of BCG magnitudes. 相似文献
158.
159.
N. Kameswara Rao V. R. Venugopal A. Patnaik 《Journal of Astrophysics and Astronomy》1985,6(3):153-157
VLA observations at 2 and 6 cm have been obtained for six hydrogen-deficient stars R CrB, HD 160641, BD — 9°4395, V348 Sgr,
MV Sgr and Sgrv Upper limits to the massloss rates have been estimated for some of these using the upper limits to the radio flux density.
National Radio Astronomy Observatory’s Very Large Array is operated by Associated Universities Inc. under contract with National
Science Foundation, USA 相似文献
160.
The gray crystalline hematite at Meridiani Planum first discovered by the Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) instrument occurs as spherules that have been interpreted as concretions. Analysis of the TES and mini-TES spectra shows that no 390 cm−1 feature is present in the characteristic martian hematite spectrum. Here, we incorporate the mid-IR optical constants of hematite into a simple Fresnel reflectance model to understand the effect of emission angle and crystal morphology on the presence or absence of the 390 cm−1 feature in an IR hematite spectrum. Based on the results we offer two models for the internal structure of the martian hematite spherules. 相似文献