全文获取类型
收费全文 | 5630篇 |
免费 | 1031篇 |
国内免费 | 1323篇 |
专业分类
测绘学 | 331篇 |
大气科学 | 1186篇 |
地球物理 | 1553篇 |
地质学 | 2731篇 |
海洋学 | 699篇 |
天文学 | 293篇 |
综合类 | 646篇 |
自然地理 | 545篇 |
出版年
2024年 | 36篇 |
2023年 | 108篇 |
2022年 | 254篇 |
2021年 | 289篇 |
2020年 | 235篇 |
2019年 | 266篇 |
2018年 | 292篇 |
2017年 | 266篇 |
2016年 | 334篇 |
2015年 | 291篇 |
2014年 | 347篇 |
2013年 | 304篇 |
2012年 | 285篇 |
2011年 | 319篇 |
2010年 | 295篇 |
2009年 | 355篇 |
2008年 | 324篇 |
2007年 | 300篇 |
2006年 | 219篇 |
2005年 | 241篇 |
2004年 | 171篇 |
2003年 | 166篇 |
2002年 | 182篇 |
2001年 | 181篇 |
2000年 | 180篇 |
1999年 | 250篇 |
1998年 | 226篇 |
1997年 | 181篇 |
1996年 | 200篇 |
1995年 | 146篇 |
1994年 | 146篇 |
1993年 | 152篇 |
1992年 | 123篇 |
1991年 | 68篇 |
1990年 | 56篇 |
1989年 | 48篇 |
1988年 | 41篇 |
1987年 | 21篇 |
1986年 | 26篇 |
1985年 | 11篇 |
1984年 | 10篇 |
1983年 | 9篇 |
1982年 | 9篇 |
1981年 | 8篇 |
1980年 | 4篇 |
1979年 | 1篇 |
1978年 | 2篇 |
1977年 | 1篇 |
1975年 | 1篇 |
1958年 | 4篇 |
排序方式: 共有7984条查询结果,搜索用时 15 毫秒
991.
应用直径26.8和4 mm两种导线平行观测的电线积冰资料,对比分析两种观测资料中电线积冰直径、厚度、重量和标准厚度的差异,并对不同天气现象和气象条件下两种电线积冰观测资料的差异进行了讨论.结果表明:总体上,2011年1-5月全国大部分台站观测的两种导线电线积冰直径、厚度和标准厚度值差异不明显,重量差异较明显,且差值较大的站点主要分布在长江以南地区;分析不同天气现象和气象条件下两种观测资料的差异后发现,两种电线积冰直径和厚度值差异在雾凇和混合凇条件下较显著,而重量值差异在雨凇、风力0~3级和气温-5~0℃的条件下时相对最大. 相似文献
992.
在人工遮雨的条件下,采用盆栽的种植方式探究"皖麦68"营养生长期(返青期—开花期)及生殖生长期(开花期—成熟期)轻度干旱胁迫(土壤相对含水量为55%±5%)及复水(土壤相对含水量为70%±5%)对其光合生理特性及产量结构的影响。结果表明:返青期至成熟期充分供水(CK)的小麦旗叶光合参数和产量最高。开花至成熟期复水(DN)的小麦叶片在复水后光合能力迅速恢复,表现出了超补偿效应:光合速率(16.43μmol/(m~2·s))甚至超过了CK(15.01μmol/(m~2·s));采用非直角双曲线模型拟合小麦旗叶的光响应曲线,其中DN的曲角θ最大;DN产量较CK略有降低但千粒重为34.51 g,高于CK(34.44 g)。开花至成熟期轻度干旱(ND)及全生育期轻度干旱(DD)的小麦光合特征参数与产量均显著降低。DD产量最低、品质最差,但其收获指数I_H高于CK、仅次于DN。在小麦返青期—开花期进行水分管理适量减少灌溉,开花期—成熟期复水能够提升籽粒的干物质积累量,获得较高的产量及品质。 相似文献
993.
Bingliang Zhuang Qian Liu Tijian Wang Changqin Yin Shu Li Min Xie Fei Jiang Huiting Mao 《Theoretical and Applied Climatology》2013,114(3-4):651-672
A Regional Climate Chemistry Modeling System that employed empirical parameterizations of aerosol-cloud microphysics was applied to investigate the spatial distribution, radiative forcing (RF), and climate effects of black carbon (BC) over China. Results showed high levels of BC in Southwest, Central, and East China, with maximum surface concentrations, column burden, and optical depth (AOD) up to 14 μg?m?3, 8 mg?m?2, and 0.11, respectively. Black carbon was found to result in a positive RF at the top of the atmosphere (TOA) due to its direct effect while a negative RF due to its indirect effect. The regional-averaged direct and indirect RF of BC in China was about +0.81 and ?0.95 W?m?2, respectively, leading to a net RF of ?0.15 W?m?2 at the TOA. The BC indirect RF was larger than its direct RF in South China. Due to BC absorption of solar radiation, cloudiness was decreased by 1.33 %, further resulting in an increase of solar radiation and subsequently a surface warming over most parts of China, which was opposite to BC’s indirect effect. Further, the net effect of BC might cause a decrease of precipitation of ?7.39 % over China. Investigations also suggested large uncertainties and non-linearity in BC’s indirect effect on regional climate. Results suggested that: (a) changes in cloud cover might be more affected by BC’s direct effect, while changes in surface air temperature and precipitation might be influenced by BC’s indirect effect; and (b) BC second indirect effect might have more influence on cloud cover and water content compared to first indirect effect. This study highlighted a substantial role of BC on regional climate changes. 相似文献
994.
对1950-2010年影响浙西南的热带气旋降水的移动路径、影响时间、强度、西风槽、西南季风以及地形等主要因子进行分析.结果表明:在玉环南-厦门一带登陆的热带气旋是影响浙西南的热带气旋中正面影响浙西南的类型,影响时间和最大平均过程降雨量、最大过程雨量存在着正相关关系,热带气旋的强度与其降水强度相关性较高.西风槽的存在不仅影响着热带气旋路径的变化,其槽前的西南气流也为热带气旋降水提供充足的水汽,同时槽后冷空气与热带气旋相结合,使丽水的西北部出现另一个强降水中心.西南季风为登陆后的热带气旋提供了水汽条件,使降水得到增幅.浙西南独特的地形,使在厦门以北到玉环以南登陆后西进、西北行或西北行后在120°E以西转向北上的热带气旋迎着山脉进入,降水强度明显加强. 相似文献
995.
996.
This paper analyses three types of artificial orbits around Mars pushed by continuous low-thrust control: artificial frozen orbits, artificial Sun-Synchronous orbits and artificial Sun-Synchronous frozen orbits. These artificial orbits have similar characteristics to natural frozen orbits and Sun-Synchronous orbits, and their orbital parameters can be selected arbitrarily by using continuous low-thrust control. One control strategy to achieve the artificial frozen orbit is using both the transverse and radial continuous low-thrust control, and another to achieve the artificial Sun-Synchronous orbit is using the normal continuous low-thrust control. These continuous low-thrust control strategies consider J 2, J 3, and J 4 perturbations of Mars. It is proved that both control strategies can minimize characteristic velocity. Relevant formulas are derived, and numerical results are presented. Given the same initial orbital parameters, the control acceleration and characteristic velocity taking into account J 2, J 3, and J 4 perturbations are similar to those taking into account J 2 perturbations for both Mars and the Earth. The control thrust of the orbit around Mars is smaller than that around the Earth. The magnitude of the control acceleration of ASFOM-4 (named as Artificial Sun-Synchronous Frozen Orbit Method 4) is the lowest among these strategies and the characteristic velocity within one orbital period is only 0.5219 m/s for the artificial Sun-Synchronous frozen orbit around Mars. It is evident that the relationship among the control thrusts and the primary orbital parameters of Martian artificial orbits is always similar to that of the Earth. Simulation shows that the control scheme extends the orbital parameters’ selection range of three types of orbits around Mars, compared with the natural frozen orbit and Sun-Synchronous orbit. 相似文献
997.
Analysis of the potential field and equilibrium points of irregular-shaped minor celestial bodies 总被引:4,自引:0,他引:4
The equilibrium points of the gravitational potential field of minor celestial bodies, including asteroids, comets, and irregular satellites of planets, are studied. In order to understand better the orbital dynamics of massless particles moving near celestial minor bodies and their internal structure, both internal and external equilibrium points of the potential field of the body are analyzed. In this paper, the location and stability of the equilibrium points of 23 minor celestial bodies are presented. In addition, the contour plots of the gravitational effective potential of these minor bodies are used to point out the differences between them. Furthermore, stability and topological classifications of equilibrium points are discussed, which clearly illustrate the topological structure near the equilibrium points and help to have an insight into the orbital dynamics around the irregular-shaped minor celestial bodies. The results obtained here show that there is at least one equilibrium point in the potential field of a minor celestial body, and the number of equilibrium points could be one, five, seven, and nine, which are all odd integers. It is found that for some irregular-shaped celestial bodies, there are more than four equilibrium points outside the bodies while for some others there are no external equilibrium points. If a celestial body has one equilibrium point inside the body, this one is more likely linearly stable. 相似文献
998.
999.
Two primary solar-activity indicators sunspot numbers(SNs)and sunspot areas(SAs)in the time interval from November 1874 to December 2012 are used to determine the chaotic and fractal properties of solar activity.The results show that(1)the long-term solar activity is governed by a low-dimensional chaotic strange attractor,and its fractal motion shows a long-term persistence on large scales;(2)both the fractal dimension and maximal Lyapunov exponent of SAs are larger than those of SNs,implying that the dynamical system of SAs is more chaotic and complex than SNs;(3)the predictions of solar activity should only be done for short-to mid-term behaviors due to its intrinsic complexity;moreover,the predictability time of SAs is obviously smaller than that of SNs and previous results. 相似文献
1000.
西天山海西中期花岗岩的地质特征及其构造环境 总被引:1,自引:0,他引:1
海西中期花岗岩是西天山加里东褶皱带内规模最大的一次岩浆活动。本文从岩石学、矿物学、岩石化学和地球化学等方面对该期花岗岩的成因类型、岩浆起源和形成的构造环境进行了探讨,认为海西中期花岗岩以I型为主,S型次之,在空间上成对分布,花岗岩浆起源于地壳;海西中期花岗岩形成于活动大陆边缘岛孤环境. 相似文献