Influences the factors of Cyclones, Anticyclones, Circulation and Rotation to the Steady Dynamic of Great Red Spot of Jupiter

Q4 Agricultural and Biological Sciences Polish Journal of Natural Sciences Pub Date : 2020-01-01 DOI:10.15640/jns.v8n2a2
A. Atai, Mahammad A.Nurmammadov
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引用次数: 2

Abstract

: In the present paper, the impact of cyclones and anticyclones phenomena on the stability of existence of the Great Red Spot on Jupiter, have been considered. In this situation, concerning all characteristically parameters, which noted by some issues of investigation, and the impact of these factors on the rotational velocity of the system of Jupiter, have been considered. For this reason, dispersion law of gravitational-gyroscopic wave, the stability of radio-waves and magneto-spherical field, magnetic energy, also mechanical coupled rotation as frictional, which effects on the solid pole (cool process) and gas-liquid pole (hot process), has been investigated by using turbulence process. The basic process of this problem solution is describing by using the mathematical model, and it is an adequate equation of motion. In this case, the new so-called terminology as a quasi-laminar with nearly zero viscose and Reynolds number, which aspires to infinity in case of turbulent transition, has been introduced. Motion equation and hydrostatic equilibrium also considered for the stability of the rotation of planetary GRS. It should be noted that, for the stability of the rotations of GRS on Jupiter, in complex form should be carried out conditions of the Rossby regime and it confirms the rotation process stability. Other hypotheses on influence factors of GRS, including structure part of the process of convection-diffusion law on Jupiter, have been considered.
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气旋、反气旋、环流和旋转因素对木星大红斑稳定动力学的影响
本文考虑了气旋和反气旋现象对木星大红斑存在稳定性的影响。在这种情况下,关于所有的特征参数,其中注意到的一些问题的调查,以及这些因素对木星系统的旋转速度的影响,已被考虑。为此,本文利用湍流过程研究了重力-陀螺波的色散规律、无线电波与磁球场的稳定性、磁能以及作为摩擦的机械耦合旋转对固体极(冷过程)和气液极(热过程)的影响。用数学模型描述了这一问题求解的基本过程,它是一个适当的运动方程。在这种情况下,引入了所谓的新术语,即具有接近零粘度和雷诺数的准层流,在湍流过渡的情况下,它渴望无穷大。考虑了行星GRS旋转稳定性的运动方程和流体静力平衡。值得注意的是,为了木星上GRS旋转的稳定性,在复杂的形式下应该进行Rossby制度的条件,它确认了旋转过程的稳定性。考虑了木星对流扩散规律过程的结构部分等对GRS影响因素的其他假设。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Polish Journal of Natural Sciences
Polish Journal of Natural Sciences Agricultural and Biological Sciences-Agricultural and Biological Sciences (all)
CiteScore
0.60
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0.00%
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0
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