全文获取类型
收费全文 | 6493篇 |
免费 | 1226篇 |
国内免费 | 1829篇 |
专业分类
测绘学 | 835篇 |
大气科学 | 1336篇 |
地球物理 | 1437篇 |
地质学 | 3192篇 |
海洋学 | 1015篇 |
天文学 | 309篇 |
综合类 | 662篇 |
自然地理 | 762篇 |
出版年
2024年 | 30篇 |
2023年 | 138篇 |
2022年 | 365篇 |
2021年 | 403篇 |
2020年 | 331篇 |
2019年 | 400篇 |
2018年 | 423篇 |
2017年 | 397篇 |
2016年 | 428篇 |
2015年 | 396篇 |
2014年 | 427篇 |
2013年 | 436篇 |
2012年 | 455篇 |
2011年 | 466篇 |
2010年 | 530篇 |
2009年 | 437篇 |
2008年 | 377篇 |
2007年 | 368篇 |
2006年 | 324篇 |
2005年 | 264篇 |
2004年 | 187篇 |
2003年 | 197篇 |
2002年 | 171篇 |
2001年 | 170篇 |
2000年 | 186篇 |
1999年 | 201篇 |
1998年 | 140篇 |
1997年 | 145篇 |
1996年 | 128篇 |
1995年 | 143篇 |
1994年 | 95篇 |
1993年 | 87篇 |
1992年 | 68篇 |
1991年 | 42篇 |
1990年 | 34篇 |
1989年 | 32篇 |
1988年 | 29篇 |
1987年 | 23篇 |
1986年 | 13篇 |
1985年 | 13篇 |
1984年 | 9篇 |
1983年 | 9篇 |
1982年 | 8篇 |
1981年 | 5篇 |
1980年 | 3篇 |
1979年 | 3篇 |
1977年 | 2篇 |
1976年 | 2篇 |
1958年 | 4篇 |
1954年 | 1篇 |
排序方式: 共有9548条查询结果,搜索用时 15 毫秒
11.
本文给出1993—1994年期间,用云南天文台1米望远镜折轴摄谱仪观测获得类太阳色球活动星。εEri的5个波段高分辨、高信噪比光谱,运用两种不同方法:谱线轮廓塞曼致宽分析和多重线统计分析法成功地测定了εEri的表面磁场强度和磁场的覆盖因子,并对这两种磁场测定方法作了简单的讨论. 相似文献
12.
LI Zhenxing LIN Hong CAO Limin 《中国海洋大学学报(英文版)》2006,5(2):115-118
The present study was undertaken to determine whether high intensity ultrasound could reduce the allergic properties of shrimp allergens. Reducing the allergenic properties of these allergens will be beneficial to allergic individuals. Samples of shrimp protein extract and shrimp muscle were treated by high-intensity ultrasound with water bathing at 0 ℃ or 50 ℃ for different time periods. The treated and untreated samples were then analyzed by SDS-PAGE, Western blots and competitive inhibition ELISA (Ci-ELISA) to determine the shrimp allergenicity. The results show that high-intensity ultrasound has no effect on allergenicity when the extracts were treated at 0℃. However, a significant decrease was observed in the level of the major shrimp allergen, Pen a 1, when the samples were treated at 50 ℃. In the determination of allergenicity with CiELISA, a reduction in IgE binding was also observed. 相似文献
13.
Boli basin, between Yishu fracture belt and Dunmi fracture belt, is the biggest Mesozoic coal basin in the east of Heilongjiang Province. Now it is a fault - fold remnant basin. The basin' s shape is generally consistent with the whole distribution of the cover folds, an arc protruding southwards. The basement of the basin can be divided into three fault blocks or structural units. The formation and evoluation of the basin in Mesozoic was determined by the basement fault blocks' displacement features rusulted from by the movement of the edge faults and the main basement faults. 相似文献
14.
We give a summary of the morphology of the two-ribbon flare of 1981 May 13. One striking feature is that the Ha flare began at about 0338' UT and the double-ribbon structure was formed about 0346, the impulsive phase of the radio 3 cm burst at 04 11 UT. The 3 cm radio burst flux beginning at 03 33 UT showed only slow, stepwise increases lasting half an hour until the impulsive phase and this type of increase is usually regarded to be a typical thermal process. Each step in the radio flux corresponded to a variation in the Ha flare, showing that the radio and Hα emissions during this period came from the same thermal source. In this paper, we explain this behaviour in terms of Hyder's model: we think that the magnetic trough supporting the solar prominence rose for some reason, causing the prominence matter (the dark filaments) to fall along the magnetic lines and to hit the chromosphere and trigger off the flare. We give rough estimates of the energy density, the height of prominence and the infall matter at the different radio increments. We also give a qualitative explanation for the appearances of the single-peak structure in the radio burst at 0411 and the covering of the sunspot shortly after at 04 13 and propose several possible mechanisms. 相似文献
15.
16.
Cao Shenglin 《Astrophysics and Space Science》1988,145(2):293-302
According to some local properties of Lorentz transformation, Einstein stated: Velocities greater than that of light have no possibility of existence. He neglected to point out the applicable range of the special theory of relativity. In fact, it could only be applied to the subluminal-speed. This paper shows that if we think of the possibility of the existence of the superluminal-speed and redescribe the special theory of relativity following Einstein's way, a new kinematic theory would be founded. The new theory would retain all kinematical meaning of the special theory of relativity when matters move with subluminal-speed and would give new content when matters move with superluminal-speed. The paper also discusses the observation principle for the motions with superluminal-speed. 相似文献
17.
Xie-Yan Song Hua-Wen Qi Paul T. Robinson Mei-Fu Zhou Zhi-Min Cao Lie-Meng Chen 《Lithos》2008,100(1-4):93-111
The Emeishan continental flood basalt (ECFB) sequence in Dongchuan, SW China comprises a basal tephrite unit overlain by an upper tholeiitic basalt unit. The upper basalts have high TiO2 contents (3.2–5.2 wt.%), relatively high rare-earth element (REE) concentrations (40 to 60 ppm La, 12.5 to 16.5 ppm Sm, and 3 to 4 ppm Yb), moderate Zr/Nb and Nb/La ratios (9.3–10.2 and 0.6–0.9, respectively) and relatively high Nd (t) values, ranging from − 0.94 to 2.3, and are comparable to the high-Ti ECFB elsewhere. The tephrites have relatively high P2O5 (1.3–2.0 wt.%), low REE concentrations (e.g., 17 to 23 ppm La, 4 to 5.3 ppm Sm, and 2 to 3 ppm Yb), high Nb/La (2.0–3.9) ratios, low Zr/Nb ratios (2.3–4.2), and extremely low Nd (t) values (mostly ranging from − 10.6 to − 11.1). The distinct compositional differences between the tephrites and the overlying tholeiitic basalts cannot be explained by either fractional crystallization or crustal contamination of a common parental magma. The tholeiitic basalts formed by partial melting of the Emeishan plume head at a depth where garnet was stable, perhaps > 80 km. We propose that the tephrites were derived from magmas formed when the base of the previously metasomatized, volatile-mineral bearing subcontinental lithospheric mantle was heated by the upwelling mantle plume. 相似文献
18.
19.
西天山达巴特矿区火山岩的形成时代、构造背景及对斑岩型矿化的制约 总被引:9,自引:0,他引:9
本文通过对西天山地区比较典型的达巴特斑岩铜钼矿床矿区范围内出露的英安岩和花岗斑岩进行了系统的岩石地球化学分析,对流纹斑岩和花岗斑岩中的锆石进行了SHRIMPU—Pb定年研究,分别获得了315.9±5.9Ma和278.7±5.7Ma。岩石化学、微量以及稀土元素特征表明从英安岩到花岗斑岩,岩体具有明显的分异演化特征和很好的继承性。火山岩和次火山岩的精确定年为准确厘定火山岩形成的时限和地球动力学背景提供了依据。结合已有的Re-Os法获得的矿化年龄,表明晚石炭世末-早二叠世初(278.7±5.7Ma),西天山地区进入板块碰撞-板内伸展阶段,由于深源岩浆侵位,在达巴特矿区形成了由花岗斑岩、流纹斑岩和流纹质角砾熔结凝灰岩组成的椭圆形火山机构,并导致相关矿床的形成。 相似文献
20.