Abstract
Abstract
Partially ionized plasma is a common occurrence in astrophysical and space environments. The emergence and development of plasma instabilities are significantly impacted by the inelastic collisions between the ions and neutrals in the partially ionized plasma, such as the charge exchange. In this study, the effect of the ion–neutral collisions on the sheared E × B flow was experimentally investigated. In the weak collision range, the shear-driven plasma instability, such as Kelvin–Helmholtz instability, was excited by the velocity-sheared flow. However, increasing ion–neutral collisions resulted in a decrease in the magnitude of the sheared E × B flow due to charge exchange–induced drag forces. Consequently, the Kelvin–Helmholtz instability is suppressed, and the Rayleigh–Taylor instability is triggered. The underlying mechanism was elucidated through experimental findings and numerical analysis. The result of this study proposes that a transition between the two modes occurred with increasing ion–neutral collision strength. It could be applied to the study of the solar chromosphere and prominence and planetary ionospheres, where plasma is partially ionized and the sheared E × B flow is often encountered.
Funder
B-type strategic priority program of Chinese Academy of Science
NSFC
the Project of Stable Support for Youth Team in Basic Research Field, CAS
Youth Innovation Promotion Association CAS
USTC Research Funds of the Double First-Class Initiative
Province Key Research and Development Program of Anhui
The Fundamental Research Funds for the Central Universities and the pre-research project on Civil Aerospace Technologies
Anhui Provincial Natural Science Foundation
Opening Foundation of CAS Key Laboratory of Geospace Environment
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
2 articles.
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