首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   7353篇
  免费   1592篇
  国内免费   2075篇
测绘学   1127篇
大气科学   1497篇
地球物理   1654篇
地质学   3646篇
海洋学   1186篇
天文学   232篇
综合类   756篇
自然地理   922篇
  2024年   48篇
  2023年   127篇
  2022年   366篇
  2021年   434篇
  2020年   377篇
  2019年   469篇
  2018年   448篇
  2017年   426篇
  2016年   435篇
  2015年   510篇
  2014年   490篇
  2013年   605篇
  2012年   590篇
  2011年   568篇
  2010年   539篇
  2009年   546篇
  2008年   525篇
  2007年   524篇
  2006年   466篇
  2005年   375篇
  2004年   262篇
  2003年   220篇
  2002年   242篇
  2001年   257篇
  2000年   209篇
  1999年   189篇
  1998年   139篇
  1997年   141篇
  1996年   99篇
  1995年   72篇
  1994年   60篇
  1993年   67篇
  1992年   55篇
  1991年   37篇
  1990年   18篇
  1989年   20篇
  1988年   11篇
  1987年   13篇
  1986年   12篇
  1985年   2篇
  1984年   6篇
  1983年   2篇
  1982年   4篇
  1981年   5篇
  1980年   2篇
  1979年   2篇
  1977年   2篇
  1958年   2篇
  1954年   2篇
排序方式: 共有10000条查询结果,搜索用时 93 毫秒
991.
Several methods of asteroid deflection have been proposed in literature and the gravitational tractor is a new method using gravitational coupling for near-Earth object orbit modification. One weak point of gravitational tractor is that the deflection capability is limited by the mass and propellant of the spacecraft. To enhance the deflection capability, formation flying solar sail gravitational tractor is proposed and its deflection capability is compared with that of a single solar sail gravitational tractor. The results show that the orbital deflection can be greatly increased by increasing the number of the sails. The formation flying solar sail gravitational tractor requires several sails to evolve on a small displaced orbit above the asteroid. Therefore, a proper control should be applied to guarantee that the gravitational tractor is stable and free of collisions. Two control strategies are investigated in this paper: a loose formation flying realized by a simple controller with only thrust modulation and a tight formation realized by the sliding-mode controller and equilibrium shaping method. The merits of the loose and tight formations are the simplicity and robustness of their controllers, respectively.  相似文献   
992.
利用多普勒频移效应,通过线宽2MHz窄线宽激光与锶原子束在大角度作用下的荧光信号分析,测量了锶原子束速率分布。比较和分析表明,理论结果与实验结果符合较好。  相似文献   
993.
Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two questions: can we distinguish the flare-induced signals from real magnetic changes during flares, and what we can learn about flare energy release from the flare-induced signals? We select the X2.6 flare that occurred on 2005 January 15, for further study. The flare took place in NOAA active re-gion (AR) 10720 at approximately the central meridian, which makes the interpretation of the vector magnetograms less ambiguous. We have identified that flare-induced signals during this flare appeared in six zones. The zones are located within an average distance of 5 Mm from their weight center to the main magnetic neutral line, have an average size of (0.6±0.4)×1017 cm2, duration of 13±4 min, and flux density change of 181±125 G in the area of reversed polarity. The following new facts have been revealed by this study: (1) the flare-induced signal is also seen in the transverse magnetograms but with smaller magnitude, e.g., about 50 G; (2) the flare-induced signal mainly manifests itself as apparent polarity reversal, but the signal starts and ends as a weakening of flux density; (3) The flare-induced signals appear in phase with the peaks of hard X-ray emission as observed by the Ramaty High Energy Solar Spectroscopic lmager (RHESSI), and mostly trace the position of RHESSI hard X-ray footpoint sources. (4) in four zones, it takes place cotemporally with real magnetic changes which persist after the flare. Only for the other two zones does the flux density recover to the pre-flare level immediately after the flare.The physical implications of the flare-induced signal are discussed in view of its relevance to the non-thermal electron precipitation and primary energy release in the flare.  相似文献   
994.
网格技术研发情况综述   总被引:1,自引:0,他引:1  
网格是继互联网的前两个浪潮Internet和Web之后的第三次浪潮,迅速受到全世界的瞩目。美国、欧洲、日本、韩国、中国等都启动了大型网格研究计划,并得到了产业界的支持。综述了各国网格技术研发情况。  相似文献   
995.
Viscosity of silicate melts is a critical property for understanding volcanic and igneous processes in the Earth. We investigate the pressure effect on the viscosity of rhyolitic melts using two methods: indirect viscosity inference from hydrous species reaction in melts using a piston cylinder at pressures up to 2.8 GPa and direct viscosity measurement by parallel-plate creep viscometer in an internally-heated pressure vessel at pressures up to 0.4 GPa. Comparison of viscosities of a rhyolitic melt with 0.8 wt% water at 0.4 GPa shows that both methods give consistent results. In the indirect method, viscosities of hydrous rhyolitic melts were inferred based on the kinetics of hydrous species reaction in the melt upon cooling (i.e., the equivalence of rheologically defined glass transition temperature and chemically defined apparent equilibrium temperature). The cooling experiments were carried out in a piston-cylinder apparatus using hydrous rhyolitic samples with 0.8-4 wt% water. Cooling rates of the kinetic experiments varied from 0.1 K/s to 100 K/s; hence the range of viscosity inferred from this method covers 3 orders of magnitude. The data from this method show that viscosity increases with increasing pressure from 1 GPa to 3 GPa for hydrous rhyolitic melts with water content ?0.8 wt% in the high viscosity range. We also measured viscosity of rhyolitic melt with 0.13 wt% water using the parallel-plate viscometer at pressures 0.2 and 0.4 GPa in an internally-heated pressure vessel. The data show that viscosity of rhyolitic melt with 0.13 wt% water decreases with increasing pressure. Combining our new data with literature data, we develop a viscosity model of rhyolitic melts as a function of temperature, pressure and water content.  相似文献   
996.
997.
磷对过铝质岩浆液相线温度影响的实验研究   总被引:2,自引:1,他引:1  
以宜春414岩体中的钠长花岗岩作为实验初始物,利用"RQV-快速内冷淬火"高温高压装置实验研究了100MPa压力、含5%H2O条件下,P对过铝质花岗岩液相线温度的影响.实验结果表明,碱性长石是最早结晶的矿物;随着体系中P2O5含量从0.27%增加到7.71%,液相线温度从最初的810℃降低到740℃,表明P有效地降低了过铝质岩浆体系的液相线温度.在过铝质岩浆体系中,P5+与Al3+的结合形成AlPO4,降低了熔体中碱性长石组分的活度,很可能是液相线温度降低的机制.  相似文献   
998.
西江干流河水主要离子及锶同位素地球化学组成特征   总被引:8,自引:1,他引:7  
水环境中锶(Sr)含量及其同位素组成特征的研究有助于认识区域水文地球化学特征及流域盆地岩石风化速率等地球化学行为,因此河流环境中Sr的地球化学行为是地球化学研究的重要课题之一。对中国南方西江干流及其支流河水主要阴阳离子及sr同位素组成进行了分析,发现其水化学组成主要以Ca^2+、Mg^2+、HCO3^-和SO4^2-离子为主,分别占阴阳离子组成的80%以上。郁江河水具有较高的Sr同位素比值(^87St/^86Sr=0.71049)和较低的Sr含量(0.0263mg/L),而西江河水具有较低的Sr同位素比值以及较高的Sr含量,其Sr含量变化范围在0.0667.0.187mg/L之间,平均含量为0.136mg/L;Sr同位素比值变化范围在0.70856.0.70936之间,平均比值为0.70894。与世界主要河流水体中Sr含量平均值(0.078mg/L)及Sr同位素比值(^87Sr/^86Sr=0.7119)相比,西江干流水体具有较高的Sr含量及较低的Sr同位素比值。两条河流河水中主要离子及Sr的来源存在显著差异,西江干流河水中的主要溶解离子及Sr同位素主要源于碳酸盐岩(石灰岩和白云岩)的风化作用,主要受黔江及其上游红水河等化学组成所控制,而郁江则主要受碎屑岩风化作用的影响;同时,中上游地区的酸沉降及人类活动的输入可能导致西江干流水体受到一定程度的污染,而郁江受污染程度则相对较小。  相似文献   
999.
金川铜镍矿床成矿模式、控矿因素分析与找矿   总被引:3,自引:0,他引:3  
高辉 《地质与勘探》2009,45(3):218-228
金川岩浆Cu-Ni-PGE硫化矿床与世界上其它几个大型硫化铜镍矿相比,具有矿化比例极高,岩体的岩相分带和矿体产状与原地熔离机制不协调等地质和成因特点.论文通过对金川铜镍矿地质构造及矿化特征、成矿模式系统分析,指出金川铜镍硫化物矿床形成和定位的主要控制因素表现为:同源岩浆控制和后期构造控制.侵入体成矿后期的构造变形对矿化的控制主要表现在对侵入体形态产状的改变,并影响到矿区深部、外围及区域矿化及分布特征,因而对矿区深部、外围及区域找矿具有指示意义.据此提出了矿区深部、外围及区域找矿新思路,并在矿床外围及区域与龙首山隆起平行的金川超镁铁岩带确定了两个勘探靶区一金川东延靶区和金川远东靶区.  相似文献   
1000.
横切潍北-莱州湾凹陷郯庐断裂带的地震反射剖面和断裂带内的凹陷断层、沉积相和油气特征,直接或间接显示了郯庐断裂带的延伸、运动性质和活动时限。郯庐断裂带在海域和陆上的几何形态及其组合基本一致,根据切过断裂带的剖面和平面上断层的组合特征,判断其为兼具垂直位移的走滑运动断层系。走滑断裂带的活动控制着凹陷内同构造沉积以及构造样式,表明郯庐断裂带的活动时限具分段性,相当于渤海湾盆地孔店组(E1?2k)-沙四段(E2?3s4)沉积期(古新世-早始新世)-孔店组-沙二段(E2?3s2)沉积期(古新世-始新世)-孔店组-沙一段(E2?3s1)(古新世-渐新世)沉积时期,走滑拉分活动由南向北迁移; 活动方式也由古新世-早始新世的左旋走滑活动,被早始新世之后的右旋走滑活动所替代。  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号