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121.
J. C. Muzzio 《Celestial Mechanics and Dynamical Astronomy》2006,96(2):85-97
We created a self-consistent triaxial stellar system through the cold disipationless collapse of 100,000 particles whose evolution was followed with a multipolar code. The resulting system rotates slowly even though its total angular momentum is zero, i.e., it offers an example of figure rotation. The potential of the system was subsequently approximated with interpolating formulae yielding a smooth potential stationary in the rotating frame. The Lyapunov exponents could then be computed for a randomly selected sample of 3,472 of the bodies that make up the system, allowing the recognition of regular and partially and fully chaotic orbits. The regular orbits were Fourier analyzed and classified using their locations on the frequency map. A comparison with a similar non-rotating model showed that the fraction of chaotic orbits is slightly but significantly enhanced in the rotating model; alternatively, there are no significant differences between the corresponding fractions neither of partially and fully chaotic orbits nor of long axis tubes, short axis tubes, boxes and boxlets among the regular orbits. This is a reasonable result because the rotation causes a breaking of the symmetry that may increase chaotic effects, but the rotation velocity is probably too small to produce any other significant differences. The increase in the fraction of chaotic orbits in the rotating system seems to be due mainly to the effect of the Coriolis force, rather than the centrifugal force, in good agreement with the results of other investigations. 相似文献
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简要介绍了三种不同旋转角下的坐标转换模型,并通过Visual C++6.0编制相应的坐标转换程序,对三种坐标转换模型的精度做对比分析,结果表明根据旋转角的大小选择不同的坐标转换模型对坐标转换精度有直接影响. 相似文献
124.
The classical problem of the critical inclination in artificial satellite theory has been extended to the case when a satellite may have an arbitrary, significant mass and the rotation momentum vector is tilted with respect to the symmetry axis of the planet. If the planet’s potential is restricted to the second zonal harmonic, according to the assumptions of the main problem of the satellite theory, two various phenomena can be observed: a critical inclination that asymptotically tends to the well known negligible mass limit, and a critical tilt that can be attributed to the effect of transforming the gravity field harmonics to a different reference frame. Stability of this particular solution of the two rigid bodies problem is studied analytically using a simple pendulum approximation. 相似文献
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地核不仅具有巨量热能,而且有巨量旋转能,这是地球能量释放的内因;天文因素使地核产生周期性的南北振荡,是地球能量间歇性释放的外因。地质旋回与天文周期直接相关,可以根据天文周期预测未来的地质变化 相似文献
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Y.-F. Yuan Jeremy S. Heyl † 《Monthly notices of the Royal Astronomical Society》2005,360(4):1493-1505
We study the evolution of a rigidly rotating protoneutron star (PNS) with hyperons and nucleons or solely nucleons in its core due to the escape of trapped neutrinos. As the neutrinos escape, the core nucleonic neutron star (NS) expands and the stellar rotation slows. After the neutrinos escape, the range of the spin periods is narrower than the initial one, but the distribution is still nearly uniform. A PNS with hyperons, at the late stage of its evolution, keeps shrinking and spinning up until all the trapped neutrinos escape. Consequently, the distribution of the stellar initial spin periods is skewed towards shorter periods. If the hyperonic star is metastable, its rotational frequency accelerates distinguishedly before it collapses to a black hole. 相似文献
130.
大气对地球自转参数(ERP)的高频激发 总被引:4,自引:0,他引:4
本文采用1983—1992年期间由空间大地测量技术观测和归算的地球自转参数(ERP)序列,以及由全球气象资料归算的大气角动量(AAM)序列,分析和研究了大气对地球自转参数的日长变化(LOD)和极移(x和y)在一个月时间尺度以内的高频激发作用,得到的主要结果如下:1大气对LOD分量高频潮汐的估计值存在着影响,但是,潮汐形变参数k/c随时间和频率的变化却是受非大气因素的扰动引起的.2.大气可以解释30天以下LOD非潮汐的大部分变化.3.极移分量30天以内的高频变化也主要由大气激发.x分量与大气的相关性要强于y分量,而且更为稳定,主要表现为平均时间尺度约为27天的波动,大气对这个波动的贡献可达70%. 相似文献