Obliquely propagating ion-acoustic solitons and supersolitons in four-component auroral plasmas

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• 作者：O.R. Rufai^a ; ^{rrufai@csir.co.za" class="auth_mail" title="E-mail the corresponding author} ; R. Bharuthram^b ; ^{rbharuthram@uwc.ac.za" class="auth_mail" title="E-mail the corresponding author} ; S.V. Singh^c ; ^{satyavir@iigs.iigm.res.in" class="auth_mail" title="E-mail the corresponding author} ; G.S. Lakhina^c ; ^{lakhina@iigs.iigm.res.in" class="auth_mail" title="E-mail the corresponding author}
• 关键词：Low frequency waves ; Solitons and supersolitons ; Magnetized plasmas ; Mach numbers ; Auroral zone ; Earth&rsquo ; s magnetosphere
• 刊名：Advances in Space Research
• 出版年：2016
• 出版时间：1 February 2016
• 年：2016
• 卷：57
• 期：3
• 页码：813-820
• 全文大小：924 K

文摘

Arbitrary amplitude nonlinear low frequency electrostatic soliton and supersoliton structures are studied in magnetized four-component auroral plasmas composed of a cold singly charged oxygen-ion fluid, Boltzmann distribution of hot protons and two distinct group of electron species. Using the Sagdeev pseudo-potential technique, the characteristics of obliquely propagating nonlinear structures are investigated analytically and numerically. The model supports the evolution of soliton and supersoliton structures in the auroral acceleration region. Depending on the parametric region, the positive and negative potential solitons coexists at lower Mach numbers, but at higher Mach numbers only negative potential solitons and supersolitons can exist. The presence of hot protons restricted the Mach number of the nonlinear structures to exist only at the subsonic region. The present investigation concurs with the Swedish Viking satellite observations in the auroral region.