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首页> 外文期刊>Doklady Earth Sciences >Structure of the Terrain and Gravitational Field of the Planets: Kaula's Rule as a Consequence of the Probability Laws by A.N. Kolmogorov and His School
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Structure of the Terrain and Gravitational Field of the Planets: Kaula's Rule as a Consequence of the Probability Laws by A.N. Kolmogorov and His School

机译:行星的地形和引力场的结构:A.N.提出的概率法则的考拉法则柯尔莫哥洛夫和他的学校

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摘要

Kaula's empirical rule has been known for more than 50 years: the coefficients of expansion over spherical harmonics for the fluctuations of the gravitational field and terrain of the planets decrease as the number of the harmonic squared. This was found for Venus, the Moon, Mars, the asteroid Vesta, and very small celestial bodies. The inverse-square line spectra were also found for various types of the Earth's surface on a scale of up to a hundred kilometers. From this it follows that the spectra of the terrain slope angles are constant, i.e., white noise. Thus, they are -correlated horizontally. These are the assumptions under which the random walk laws were derived by A.N. Kolmogorov in 1934. Using them, the equation of the horizontal probability diffusion of the terrain with the linear coefficient of diffusion D is derived. Based on the empirical data, D = 1.3 +/- 0.3 m for the Earth, while for Venus it is almost an order of magnitude less. The slopes resist the wind; the rock crumbles, and the water flows down the slopes as well. This consideration turns Kuala's rule into the random walk laws (over terrain) developed by Kolmogorov in 1934.
机译:考拉(Kaula)的经验法则已经有50多年的历史了:随着引力平方的平方,随着重力场和行星地形的波动,球形谐波的膨胀系数减小。这是为金星,月亮,火星,小行星维斯塔和非常小的天体发现的。还发现了各种类型的地球表面的平方平方线谱,其尺度可达一百公里。由此可知,地形倾斜角的频谱是恒定的,即白噪声。因此,它们在水平方向上相关。这些是A.N.得出随机游走定律的假设。 1934年Kolmogorov。利用它们,得出了线性扩散系数为D的地形的水平概率扩散方程。根据经验数据,地球D = 1.3 +/- 0.3 m,而对于金星,D几乎小一个数量级。斜坡抵抗风;岩石崩溃了,水也顺着山坡流了下来。这种考虑将瓜拉的规则变成了由科尔莫戈罗夫(Kolmogorov)在1934年制定的随机行走定律(越过地形)。

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  • 来源
    《Doklady Earth Sciences》 |2019年第2期|391-394|共4页
  • 作者

    Gledzer E. B.; Golitsyn G. S.;

  • 作者单位

    Russian Acad Sci, Obukhov Inst Atmospher Phys, Moscow 119017, Russia;

    Russian Acad Sci, Obukhov Inst Atmospher Phys, Moscow 119017, Russia;

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