Plane Internal Gravity Waves with Arbitrary Amplitude

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
O. K. Cheremnykh, S. O. Cheremnykh, V. M. Lashkin, A. K. Fedorenko
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引用次数: 0

Abstract

Nonlinear equations called the Stenflo equations are usually used for the analytical description of the propagation of internal gravity waves in the Earth’s upper atmosphere. Solutions in the form of dipole vortices, tripole vortices, and vortex chains are previously obtained by these equations. The Stenflo equations also describe rogue waves, breathers, and dark solitons. If disturbances cease to be small, then their profiles are usually deformed, and, presumably, they cannot be considered plane waves. This study shows that this is not always the case for internal gravity waves and that these waves can propagate as plane waves even with large amplitudes. An exact solution of the system of nonlinear Stenflo equations for internal gravity waves that contain nonlinear terms in the form of Poisson brackets is given. The solution is obtained in the form of plane waves with arbitrary amplitude. To find a solution, the original system of equations is transformed. It is split into equations for the stream and vorticity functions as well as equations for the perturbed density. To solve the obtained equations, the procedure of the successive zeroing of Poisson brackets is applied. As a result, linear equations that allow one to find the accurate analytical solutions for internal gravity waves in the form of plane waves with arbitrary amplitude are obtained. By solving these linear equations in two different ways, we have analytically found expressions for the perturbed quantities and the dispersion equation. The nonlinear equations obtained for the current, vorticity, and perturbed density functions can be used to find other nonlinear solutions. The given solutions in the form of plane waves with arbitrary amplitude may be of interest for the analysis of the propagation of internal gravity waves in the Earth’s atmosphere and the interpretation of experimental data.

具有任意振幅的平面内部重力波
被称为斯登弗洛方程的非线性方程通常用于分析描述地球高层大气中内部重力波的传播。这些方程曾得到偶极涡旋、三极涡旋和涡旋链等形式的解决方案。斯登弗洛方程还描述了流氓波、呼吸器和暗孤子。如果扰动不再是小的,那么它们的轮廓通常会变形,因此不能被视为平面波。本研究表明,内引力波的情况并非总是如此,这些波即使振幅很大,也可以作为平面波传播。本文给出了内重力波非线性 Stenflo 方程系统的精确解,该方程包含泊松括号形式的非线性项。解以任意振幅的平面波形式获得。为了找到解,需要对原始方程组进行转换。它被拆分为流和涡度函数方程以及扰动密度方程。为了求解所得到的方程,采用了泊松括号连续归零的程序。结果,得到了线性方程,可以找到任意振幅平面波形式的内部重力波的精确分析解。通过用两种不同的方法求解这些线性方程,我们通过分析找到了扰动量和频散方程的表达式。电流、涡度和扰动密度函数的非线性方程可用于寻找其他非线性解。以任意振幅的平面波形式给出的解可能对分析地球大气层内部重力波的传播和解释实验数据有意义。
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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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