Nonlinear ion-acoustic waves at Venus ionosphere

被引：17

作者：

Sayed, F. S. H. ^{[1
]}

Turky, A. A. ^{[1
]}

Koramy, R. A. ^{[1
]}

Moslem, W. M. ^{[2
,3
]}

机构：

[1] Assiut Univ, Fac Sci, Dept Phys, Asyut 71516, Egypt

[2] Port Said Univ, Fac Sci, Dept Phys, Port Said 42521, Egypt

[3] British Univ Egypt, Ctr Theoret Phys, Cairo, Egypt

来源：

ADVANCES IN SPACE RESEARCH | 2020年 / 66卷 / 06期

关键词：

Ion-acoustic waves; Venus ionosphere; Solitons; Sagdeev pseudo-potential; Mach number; SOLAR-WIND INTERACTION; SOLITARY WAVES; PLASMA; SOLITONS; PROPAGATION; DYNAMICS;

D O I：

10.1016/j.asr.2020.06.023

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

High altitude Venus ionosphere is characterized by the presence of H+ and O+ ions as well as electrons. Because of these two positive ions, the ion-acoustic wave (IAW) was observed. Propagation properties of nonlinear IAWs in the Venusian ionosphere are investigated. Korteweg de-Vries (KdV) equation is derived for weakly nonlinear behavior of the IAWs, while Sagdeev pseudo-potential is obtained to study an arbitrary amplitude IAWs. The region for the lower and upper limits of Mach number for the existence of soliton structures are determined. The physical parameters, such as density and temperature ratios, are investigated on the profiles of both weakly and fully nonlinear waves. Furthermore, subsonic waves can exist in the lower ionosphere whereas supersonic waves propagate at higher altitude. This is in good agreement with the observations. (C) 2020 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：1276 / 1285

页数：10

共 35 条

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