Fluid theory and kinetic simulation of two-dimensional electrostatic streaming instabilities in electron-ion plasmas

NCUIR > College of Earth Sciences > DEPARTMENT OF SPACE SCIENCE AND ENGINEERING > journal & Dissertation > Item 987654321/102193

Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/102193

Title:	Fluid theory and kinetic simulation of two-dimensional electrostatic streaming instabilities in electron-ion plasmas
Authors:	郝玲妮;Jao, C.-S.;Hau, L.-N.
Contributors:	地球科學學院太空科學與工程學系
Keywords:	Electron mass;Electrons;Evolution;Kinetic theory;Magnetic fields;Plasma physics;Simulation;Solitary waves;Space plasmas;Stability
Date:	2016-11-01
Issue Date:	2026-04-23 11:03:57 (UTC+8)
Publisher:	American Institute of Physics;Melville: AIP Publishing
Abstract:	摘要： Electrostatic streaming instabilities have been proposed as the generation mechanism for the electrostatic solitary waves observed in various space plasma environments. Past studies on the subject have been mostly based on the kinetic theory and particle simulations. In this paper, we extend our recent study based on one-dimensional fluid theory and particle simulations to two-dimensional regimes for both bi-streaming and bump-on-tail streaming instabilities in electron-ion plasmas. Both linear fluid theory and kinetic simulations show that for bi-streaming instability, the oblique unstable modes tend to be suppressed by the increasing background magnetic field, while for bump-on-tail instability, the growth rates of unstable oblique modes are increased with increasing background magnetic field. For both instabilities, the fluid theory gives rise to the linear growth rates and the wavelengths of unstable modes in good agreement with those obtained from the kinetic simulations. For unmagnetized and weakly magnetized systems, the formed electrostatic structures tend to diminish after the long evolution, while for relatively stronger magnetic field cases, the solitary waves may merge and evolve to steady one-dimensional structures. Comparisons between one and two-dimensional results are made and the effects of the ion-to-electron mass ratio are also examined based on the fluid theory and kinetic simulations. The study concludes that the fluid theory plays crucial seeding roles in the kinetic evolution of electrostatic streaming instabilities. 出版者： Melville: AIP Publishing 出版日期： 2016-11-01 出處： Physics of Plasmas, 2016-11, Vol.23 (11) 資源來源： AIP Journals (American Institute of Physics) 版權： Author(s) 版權： 2016 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/). 識別號： ISSN: 1070-664X 識別號： ISSN: 1527-2419 識別號： ISSN: 1089-7674 識別號： EISSN: 1089-7674 識別號： DOI: 10.1063/1.4967283 識別號： CODEN: PHPAEN
Appears in Collections:	[DEPARTMENT OF SPACE SCIENCE AND ENGINEERING] journal & Dissertation

Files in This Item:

File	Description	Size	Format
index.html		0Kb	HTML	32	View/Open

社群 sharing

Loading...