Динамические эффекты во вращении Земли, вызванные годовыми и полугодовыми циклическими перераспределениями масс планеты

Array Ю. Баркин
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Abstract

The paper deals with development of the theory of perturbed rotational motion of a celestial body with variable geometry of the masses. Its main task is to study the impact of annual and semi-annual variations of the Earth's mass geometry (a component of its inertia tensor), as well as a component of its relative angular momentum, on the movement of the Earth's poles and its axial rotation. The body is considered to be a free (isolated), and the problem formulation corresponds to the classical Liouville problem on rotation of a variable body. Euler conical movement of the axially symmetric body with an arbitrary constant half-angle  is assumed as the unperturbed motion. In the classical theory of the Earth's rotation this angle is usually assumed to be zero. In the last 20 years, accuracy to determine the Earth rotation parameters owing to using methods of space geodesy and method of Very Long Baseline Interferometry (VLBI) has increased by about three orders of magnitude and has made about  i.e., in angle measure it is about 10 - 20 arc-microseconds. According to experts, the theory of the Earth's rotation with such precision is not created yet. The paper is focused just on the new dynamic studies of the Earth rotation at a higher level of accuracy than has been done in previous studies, using a new approach to the problem, based on the new forms of the equations of motion (in the Andoyer variables) and the analytical methods of perturbation theory (small parameter method). The problem of perturbed rotational motion with variable geometry and variable mass relative angular momentum in the first approximation is solved in Andoyer variables and projections of the angular velocity of the planet rotation. The analytical solution allows us to run applications to study dynamic effects from above factors for various bodies in the solar system, including the Earth. The solution allowed us to obtain the following parameters of the fundamental effects in the Earth's rotation: the annual and semi-annual fluctuations of the axis pole of Earth's rotation, annual and semiannual variations in the axial Earth's rotation. The theoretical values of the parameters are in good agreement with modern observation data of the Earth's rotation and the cyclical variations in the geo-potential coefficients.
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地球每年和6个月的周期性行星质量再分配对地球自转的动态影响
本文讨论了具有变几何质量的天体的微扰旋转运动理论的发展。它的主要任务是研究地球质量几何(它的惯性张量的一个分量)的年度和半年度变化,以及它的相对角动量的一个分量,对地球的两极运动和轴向旋转的影响。该体被认为是自由的(孤立的),问题的形式对应于经典的关于变体旋转的刘维尔问题。假定轴对称体具有任意恒定半角的欧拉圆锥运动为无摄动运动。在地球自转的经典理论中,这个角度通常被假定为零。近20年来,利用空间大地测量法和甚长基线干涉测量法测定地球自转参数的精度提高了约3个数量级,测角精度约为10 - 20弧微秒。据专家称,如此精确的地球自转理论还没有被创造出来。本文的重点是在新的运动方程形式(在Andoyer变量中)和摄动理论的分析方法(小参数方法)的基础上,使用一种新的方法,在比以前的研究更高的精度上对地球自转进行新的动力学研究。利用行星旋转角速度的安多耶变量和投影,解决了一阶近似中具有变几何和变质量相对角动量的摄动旋转运动问题。解析解允许我们运行应用程序来研究上述因素对包括地球在内的太阳系中各种天体的动态影响。这个解使我们能够得到下列关于地球自转基本影响的参数:地球旋转轴极的年度和半年度波动,地球旋转轴的年度和半年度变化。这些参数的理论值与地球自转和地势系数周期性变化的现代观测资料吻合较好。
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Исследование эффективности мульти-меметического алгоритма эволюции разума Динамические эффекты во вращении Земли, вызванные годовыми и полугодовыми циклическими перераспределениями масс планеты
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