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121.
Adam Ružčka 《Astrophysics and Space Science》2003,284(2):519-522
A simple sticky-particle numerical model has been developed in order to check whether extended structures of gas created due
to the dynamical evolution of the Galaxy and the Magellanic Clouds system can be explained as remnants of a tidal interaction.
Influence of dissipative nature of gaseous medium has been taken into account. The most remarkable features are: the Magellanic
Stream, the common HI envelope surrounding both the LMC and SMC and the bridge extended between the Clouds. In contrast to
previous works of Murai and Fujimoto (1980), Gardiner et al. (1994) and H and Rohlfs (1994) no presumptions were done on the
actual galactocentric velocities of the Magellanic Clouds. The mean values of the LMC and SMC velocity vectors obtained from
the Hipparcos proper motion measurements (Kroupa and Bastian, 1997) were used in order to verify whether they allow to reproduce
the observed HI distribution. Numerical simulations showed that tidal forces are really significant for the evolution of extended
structures such as the Magellanic Stream but this approach becomes unsufficient for the internal regions of galaxies where
self-gravity and dissipative properties of the gas cannot be neglected. More precise proper motion measurements are urgently
needed.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
122.
At times of strong solar wind forcing such as those that produce major magnetic storms, the region 1 current system dominates over the Chapman–Ferraro current system in mediating the transfer of force between the solar wind and the terrestrial system. The global force balance can be broken into two components, one involving the high-altitude part of the region 1 current system that is in contact with the solar wind (labeled here the HRS) and the other involving the low-altitude part of the region 1 current system that lies in the ionosphere (the LRS). Both communicate their J×B force to the geomagnetic dipole via a gradient in the magnetic field that they generate. In the HRS case the force acts to push the dipole away from the sun. This is the region 1 analog of the Chapman–Ferraro mechanism for transmitting the solar wind's force to the Earth. However, in the LRS case, the force (which is much stronger than in the HRS case) acts to push the dipole toward the sun, seemingly paradoxically. The LRS balances the ‘paradoxical’ sunward force on the dipole with an opposite force on the atmosphere. This paper uses MHD simulations to demonstrate the presence of both the normal force-transmitting gradient generated by the Chapman–Ferraro and the counter-Chapman–Ferraro gradient in the magnetic field generated by the region 1 current system. 相似文献
123.
就目前锚索抗滑桩的研究现状来看,基本上都是将锚索和抗滑桩分开计算,忽略了锚索与抗滑桩之间存在的相互作用关系。针对这一问题,对锚索-抗滑桩-岩土体相互作用系统的计算方法进行了研究。提出了在锚索抗滑桩设计计算中,除了应考虑锚索的强度外。还应该考虑锚索的伸长量,使其与桩的变形相协调。在此基础上,建立了新的锚索抗滑桩计算理论。本文用该方法进行了工程实例分析,并与其他计算方法所得结果进行了对比。 相似文献
124.
2004年9月2—6日四川盆地中东部发生了一次持续性强暴雨过程。利用时间平均合成分析方法对强暴雨维持期间 (9月3日20:00—5日08:00, 北京时) 的探测资料进行合成平均, 再对合成平均资料做诊断分析, 以揭示持续性强暴雨过程持续期的平均特征。诊断分析显示, 台风西进导致稳定的环流以及中低层大量的水汽输送为暴雨持续提供了背景条件。在时间平均流场上, 与暴雨相联系的中尺度系统十分显著, 它在对流层中低层表现为准东西向的中尺度辐合带, 在对流层高层表现为中尺度辐散带, 两者垂直耦合为深厚系统。此外, 在暴雨持续期间, 对流层低层大气运动表现出强烈的非平衡特征, 这种非平衡的动力强迫作用支撑着低层强辐合的维持。 相似文献
125.
126.
Vyacheslav M. Zobin Carlos J. Navarro-Ochoa Gabriel A. Reyes-Dávila 《Bulletin of Volcanology》2006,69(2):141-147
In July–August 2003, the andesitic lava dome at Volcán de Colima, México, was destroyed by a sequence of explosions that replaced the 2×106 m3 dome with a crater 200 m across and 30 m deep. The two strongest explosions occurred on July 17 and August 28. The initial low-frequency impulses that they produced, which were recorded on broadband seismic records, allowed an estimation of the counter forces of the initiating process as being equal to 0.3×1011 N and 1×1011 N for the July and August events, respectively. The seismic characteristics follow the Nishimura-Hamaguchi scaling law for volcanic explosions, reflecting self-similarity in the processes initiating explosive events. The results also show that counter forces can discriminate between the sizes of explosive eruptions that are assigned the same magnitude by conventional methods of classification such as the Volcanic Explosivity Index. The increasing use of broadband seismometers may therefore provide the basis for using counter forces to determine the magnitude of explosive eruptions. 相似文献
127.
128.
129.
A Combined-Power Model for the Distribution of Axial Force in Shaft Anchor along Its Length 总被引:1,自引:0,他引:1
INTRODUCTIONThe anchorage of geomaterial , including shaftanchors and prestressed tendons ,is usually used ingeotechnical engineering. Owing to various advanta-ges ,these two anchorage types are widely used instructures in China ( Cao et al ., 2003 ; Fu et al .,1999 ;Lu et al .,1998 ; Li et al .,1995) . Shaft an-chors can be classifiedinto three kinds by the forceinthe shaft and cement grout :tensile ,press ,and sheartype (Lu et al .,1998) . The tensile type is the mostpopular in China… 相似文献
130.
利用塔中气象站1997—2002年的气象资料, 从沙尘源丰富程度、风动力条件和空气稳定度等方面分析了塔克拉玛干沙漠腹地沙尘暴的成因。结果表明:在塔克拉玛干沙漠腹地, 沙尘源极为丰富, 为沙尘暴发生提供了必要条件, 降水基本不能改变沙面的湿润状况, 沙尘源丰富度不是沙尘暴发生的限制因子; 风动力是沙尘暴发生的重要条件, 而月平均风速和大风日数是风动力的重要定量表征指标; 空气稳定性也是沙尘暴发生的重要条件, 温度和天气过程是其重要标志, 沙尘暴发生与温度呈正相关, 沙尘暴多发生在夏季和午后; 降水是沙漠腹地天气过程的重要指标, 月降水日数和降水总量与沙尘暴日数呈正相关; 20世纪90年代以来沙尘暴逐年减少, 这种变化趋势可能与全球气候变化有关。 相似文献