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61.
The rapid rotation of the gas giant planets, Jupiter and Saturn, leads to the formation of magnetodisc regions in their magnetospheric environments. In these regions, relatively cold plasma is confined towards the equatorial regions, and the magnetic field generated by the azimuthal (ring) current adds to the planetary dipole, forming radially distended field lines near the equatorial plane. The ensuing force balance in the equatorial magnetodisc is strongly influenced by centrifugal stress and by the thermal pressure of hot ion populations, whose thermal energy is large compared to the magnitude of their centrifugal potential energy. The sources of plasma for the Jovian and Kronian magnetospheres are the respective satellites Io (a volcanic moon) and Enceladus (an icy moon). The plasma produced by these sources is globally transported outwards through the respective magnetosphere, and ultimately lost from the system. One of the most studied mechanisms for this transport is flux tube interchange, a plasma instability which displaces mass but does not displace magnetic flux—an important observational constraint for any transport process. Pressure anisotropy is likely to play a role in the loss of plasma from these magnetospheres. This is especially the case for the Jovian system, which can harbour strong parallel pressures at the equatorial segments of rotating, expanding flux tubes, leading to these regions becoming unstable, blowing open and releasing their plasma. Plasma mass loss is also associated with magnetic reconnection events in the magnetotail regions. In this overview, we summarise some important observational and theoretical concepts associated with the production and transport of plasma in giant planet magnetodiscs. We begin by considering aspects of force balance in these systems, and their coupling with the ionospheres of their parent planets. We then describe the role of the interaction between neutral and ionized species, and how it determines the rate at which plasma mass and momentum are added to the magnetodisc. Following this, we describe the observational properties of plasma injections, and the consequent implications for the nature of global plasma transport and magnetodisc stability. The theory of the flux tube interchange instability is reviewed, and the influences of gravity and magnetic curvature on the instability are described. The interaction between simulated interchange plasma structures and Saturn’s moon Titan is discussed, and its relationship to observed periodic phenomena at Saturn is described. Finally, the observation, generation and evolution of plasma waves associated with mass loading in the magnetodisc regions is reviewed.  相似文献   
62.
利用显式非线性有限元方法对薄壁圆柱筒轴向载荷下的动力学响应进行了研究,模拟了圆柱筒在轴向冲击作用下的动力屈曲变形及其发展过程。分析比较了不同单元尺度下冲击模型的数值计算解与理论解,揭示了在进行有限元模拟时存在的网格尺寸效应,为研究有限元网格尺寸与有限元求解精度的内在联系提供参考;为在保证数值解满足工程实际精度要求的前提下,确定合理的单元尺度,提高有限元分析效率进行了有益的探索。  相似文献   
63.
论文通过对桂林航天工业高等专科学校部分学生的英语学习策略调查问卷及相关数据进行SPSS数据分析,分析通过大学英语四级的学生英语学习策略使用情况,及通过分析调查对象的英语学习策略使用情况,是否知道学习策略对于学习策略的选择的影响,各学习策略之间的关系等提出,指导学生,提高大学英语四级通过率。  相似文献   
64.
为了定量描述空域扇区的复杂性,引入交通内禀性概念,通过计算扇区内航空器间的逼近时间、侵略函数、关系矩阵、相关度函数,建立扇区的复杂性测度模型;并通过仿真算例,对扇区复杂度影响因素进行了分析.研究结果表明:复杂性值大小反映了扇区内飞机数量及汇聚、分散程度,复杂性值曲线拐点数量反映了扇区交通有序/无序程度,复杂性值曲线突变反映了扇区交通数量变化情况,可为管制员的监视和冲突解脱方案选择提供一定支持.  相似文献   
65.
Using Atmospheric Infrared Sounder (AIRS) products of atmospheric temperature and geopotential height, we investigate the atmospheric response to HE0611, which was found and investigated by [Qin, H., Kawamura, H., Sakaida, F., Ando, K. A case study of the tropical Hot Event in November 2006 (HE0611) using a geostationary meteorological satellite and the TAO/TRITON mooring array. J. Geophys. Res. 113, C08045, doi: 10.1029/2007JC004640, 2008]. HE0611 was formed by connecting two very high SST areas, HE0611-East and HE0611-West. The period-mean atmosphere temperatures at levels of 925 and 850 hPa in HE0611-West are higher, by about 0.5 K, than those in WE0611-East while the atmospheric temperatures at middle to high levels (700–300 hPa) are higher in HE0611-East. The period-mean geopotential heights HE0611-East are much lower than those in HE0611-West for the levels from the surface to 400 hPa. The mean geopotential heights from 400 hPa to 200 hPa are higher in HE0611-East. In the middle and high layers over HE0611-West, the atmosphere temperatures gradually decrease from 7th to 17th, and then increase significantly. The increase in HE0611-East starts from 15th November, which is earlier than that of HE0611-West. The geopotential heights in the high layer of both the areas also show corresponding behaviors. The lagged atmospheric response in the western part is confirmed by the correlation analysis. It emerges that the atmospheric response to HE0611 is well organized and associated with deep convention in HE0611-East and subsidence in HE0611-West. These are also consistent with the HE0611 features and evolution revealed by earlier HE studies.  相似文献   
66.
In this paper, a brief review and generalization of studies on the heat transfer and heat conduction problem in a variable domain are presented. The equations of the process, where the boundary displacement velocity is the control, are obtained taking into account heat inflow. This article was submitted by the authors in English.  相似文献   
67.
本文利用 Tutte 定理,给出并证明了满足一定条件的2k 1正则图中的每个边都是自由边的结论。  相似文献   
68.
格栅翼减阻特性研究   总被引:1,自引:0,他引:1  
为了探索减少格栅翼阻力的方法和途径 ,进行了超声速M∞ =2 .5 2 1下格栅翼的边框几何形状和尺寸以及格栅翼茎厚度、格栅几何形状对格栅翼阻力特性影响的风洞实验。结果显示 ,格栅翼的边框对格栅翼的阻力影响最大 ,选择合适的边框厚度和剖面形状可以有效地减少格栅翼的阻力  相似文献   
69.
1998年夏天,暑热正浓的日子,我走进好友萧缤在红瓦寺那间有些沧桑的欧式风格的画室,照例是饮点小酒然后挥毫。当时的萧缤正在省诗书画院进修,师从秦天柱。那时我刚从深圳归来不久,对四川的化艺术界并不是太熟悉,第一次见到那般生动空灵的花鸟画,被画面上扑面而来的诗般的意象所打动,时时临写,记忆犹新。后来虽然中断了绘画,仍然很关注先生的作品,时不时在一些报刊和画集中见到那些打动人心灵的画作。遗憾的是一直无缘与这位才华横溢的画家谋面,但其作品自然流露出的恬淡与闲适高雅之气直相伴我走过高原丘陵和平原。  相似文献   
70.
用电火花加工复杂形状模腔的关键之一是工具电极的制造。为了解决一般电极材料价高,复杂型腔难以加工等问题,通过试验研究,推出了一种以石膏和塑料为基本材料,采用非金属电镀工艺制造工具电极的新方法。  相似文献   
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