{"title":"Ion Acoustic Shock Waves with Nonextensive Electron Distributions in a Five-Component Cometary Plasma","authors":"N. T. Willington, C. Venugopal","doi":"10.3103/S1541308X25700098","DOIUrl":null,"url":null,"abstract":"<p>This work analyzes ion-acoustic shock waves in the presence of an external noise or perturbation by deriving the Korteweg–de Vries–Burgers–Kuramoto (KdVBK) equation. Our plasma model is a five-component magnetized, temperature anisotropic, cometary plasma consisting of two components of electrons (of solar and cometary origin) described by nonextensive distribution functions, a drifting ion component (H<sub>3</sub>O<sup>+</sup>) and a pair of oppositely charged oxygen ion components. We have studied the solution of the KdVBK equation in the vicinity of the “inner shock” that occurred at a cometocentric distance of roughly 4000 km for comet 1P/Halley. A drop in the shock amplitude is observed with an increase in the nonextensive parameter of the electrons and as the temperature of the cometary electrons rise. It is found that a shock wave oriented perpendicular to the direction of the magnetic field dissipates more quickly than one that is parallel. As the values of the parallel pressures of H<sub>3</sub>O<sup>+</sup>, O<sup>+</sup> and O<sup>−</sup> ions increase, the shock amplitude reduces. The dissipation coefficient <i>C</i> is found to rise with increasing kinematic viscosities of ions. Additionally, the shock amplitude exhibits a direct correlation with the ambient magnetic field strength. Also, in general, the shock amplitudes are slightly greater when described by the KdVBK equation rather than the KdVB equation.</p>","PeriodicalId":732,"journal":{"name":"Physics of Wave Phenomena","volume":"33 2","pages":"146 - 158"},"PeriodicalIF":1.1000,"publicationDate":"2025-05-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics of Wave Phenomena","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.3103/S1541308X25700098","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
This work analyzes ion-acoustic shock waves in the presence of an external noise or perturbation by deriving the Korteweg–de Vries–Burgers–Kuramoto (KdVBK) equation. Our plasma model is a five-component magnetized, temperature anisotropic, cometary plasma consisting of two components of electrons (of solar and cometary origin) described by nonextensive distribution functions, a drifting ion component (H3O+) and a pair of oppositely charged oxygen ion components. We have studied the solution of the KdVBK equation in the vicinity of the “inner shock” that occurred at a cometocentric distance of roughly 4000 km for comet 1P/Halley. A drop in the shock amplitude is observed with an increase in the nonextensive parameter of the electrons and as the temperature of the cometary electrons rise. It is found that a shock wave oriented perpendicular to the direction of the magnetic field dissipates more quickly than one that is parallel. As the values of the parallel pressures of H3O+, O+ and O− ions increase, the shock amplitude reduces. The dissipation coefficient C is found to rise with increasing kinematic viscosities of ions. Additionally, the shock amplitude exhibits a direct correlation with the ambient magnetic field strength. Also, in general, the shock amplitudes are slightly greater when described by the KdVBK equation rather than the KdVB equation.
期刊介绍:
Physics of Wave Phenomena publishes original contributions in general and nonlinear wave theory, original experimental results in optics, acoustics and radiophysics. The fields of physics represented in this journal include nonlinear optics, acoustics, and radiophysics; nonlinear effects of any nature including nonlinear dynamics and chaos; phase transitions including light- and sound-induced; laser physics; optical and other spectroscopies; new instruments, methods, and measurements of wave and oscillatory processes; remote sensing of waves in natural media; wave interactions in biophysics, econophysics and other cross-disciplinary areas.