全文获取类型
| 收费全文 | 13275篇 |
| 免费 | 1799篇 |
| 国内免费 | 2803篇 |
专业分类
| 测绘学 | 646篇 |
| 大气科学 | 642篇 |
| 地球物理 | 1857篇 |
| 地质学 | 6995篇 |
| 海洋学 | 1287篇 |
| 天文学 | 5134篇 |
| 综合类 | 612篇 |
| 自然地理 | 704篇 |
出版年
| 2024年 | 40篇 |
| 2023年 | 132篇 |
| 2022年 | 305篇 |
| 2021年 | 332篇 |
| 2020年 | 383篇 |
| 2019年 | 469篇 |
| 2018年 | 403篇 |
| 2017年 | 357篇 |
| 2016年 | 406篇 |
| 2015年 | 441篇 |
| 2014年 | 748篇 |
| 2013年 | 792篇 |
| 2012年 | 826篇 |
| 2011年 | 959篇 |
| 2010年 | 958篇 |
| 2009年 | 1296篇 |
| 2008年 | 1172篇 |
| 2007年 | 1084篇 |
| 2006年 | 1039篇 |
| 2005年 | 904篇 |
| 2004年 | 785篇 |
| 2003年 | 663篇 |
| 2002年 | 547篇 |
| 2001年 | 484篇 |
| 2000年 | 422篇 |
| 1999年 | 402篇 |
| 1998年 | 335篇 |
| 1997年 | 181篇 |
| 1996年 | 175篇 |
| 1995年 | 132篇 |
| 1994年 | 133篇 |
| 1993年 | 130篇 |
| 1992年 | 67篇 |
| 1991年 | 62篇 |
| 1990年 | 58篇 |
| 1989年 | 31篇 |
| 1988年 | 33篇 |
| 1987年 | 24篇 |
| 1986年 | 29篇 |
| 1985年 | 32篇 |
| 1984年 | 20篇 |
| 1983年 | 18篇 |
| 1982年 | 17篇 |
| 1981年 | 7篇 |
| 1980年 | 12篇 |
| 1979年 | 3篇 |
| 1978年 | 7篇 |
| 1977年 | 15篇 |
| 1877年 | 1篇 |
| 1875年 | 1篇 |
排序方式： 共有10000条查询结果，搜索用时 638 毫秒
81.
The absolute magnitudeM
v
of the hydrogen deficient binary υ Sgr has been estimated as -4.8 ± 1.0 from the distribution of the interstellar reddening,
polarization and interstellar lines of the surrounding stars. From the ANS observations obtained at the time of the secondary
eclipse, it appears that the hotter secondary is surrounded by a disc with colours of a B8-B9 star. The λ 1550 CIv absorption
line arising in the stellar wind does not show any change in strength during the secondary minimum. The upper limit to the
mass-loss rate from the high temperature wind is estimated as ≤ 5 × 10-7 M⊙ yr-1 from the 2 cm and 6 cm radio observations.
Based on observations obtained with the Astronomical Netherlands Satellite and VLA. The National Radio Astronomy Observatory’s
Very Large Array at Socorro, New Mexico is operated by Associated Universities Inc. under contract with the National Science
Foundation. 相似文献
82.
秦岭凤太矿田层控铅锌(铜)矿床的金属物质、硫和成矿溶液主要来自深部基底的岩石,属海底喷流—沉积成因矿床。从这一理论认识出发可进一步分析控矿地质条件及今后在该区有效地寻找同类矿床。 相似文献
83.
84.
85.
We present a new Very Large Array (VLA) image of Saturn, made from data taken in October 1998 at a wavelength of λ3.6 cm. The moderate ring opening angle (B≈15°) allows us to explore direct transmission of microwave photons through the A and C rings. We find a strong asymmetry of photons transmitted through the A ring, but not in the C ring, a new diagnostic of wake structure in the ring particles. We also find a weak asymmetry between east and west for the far side of the ansae. To facilitate quantitative comparison between dynamic models of the A ring and radio observations, we extend our Monte Carlo radiative transfer code (described in Dunn et al., 2002, Icarus 160, 132-160) to include idealized wakes. We show the idealized model can reproduce the properties of dynamic simulations in directly transmitted light. We examine the model behavior in directly transmitted and scattered light over a range of physical and geometric wake parameters. Finally, we present a wake model with a plausible set of physical parameters that quantitatively reproduces the observed intensity and asymmetry of the A ring both across the planet and in the ansae. 相似文献
86.
87.
88.
89.
R. F. Griffin 《Journal of Astrophysics and Astronomy》1990,11(4):533-540
Photoelectric radial-velocity measurements show that HD 118670 is a double-lined spectroscopic binary in an orbit which is
not quite circular and whose period is about 48 days. Spectral types of K0 V and K7 V would satisfy the photometry and the
mass ratio; the mass function would then suggest the possibility of eclipses. However, actual spectral classification indicates
a luminosity somewhat above the main sequence 相似文献
90.