On the tearing instability of highly elongated current sheets
Grigory Vekstein

TL;DR
This paper demonstrates how the main results of the complex tearing instability theory can be reproduced through a simple qualitative analysis of MHD equations, making the concepts more accessible.
Contribution
It introduces a straightforward qualitative approach to understanding the tearing instability in highly elongated current sheets, simplifying the complex mathematical theories.
Findings
Main results reproduced by qualitative analysis
Simplified understanding of tearing instability
Accessible approach to complex MHD theories
Abstract
Rigorous theories of the tearing instability are mathematically quite involving. Therefore, the present note aims to demonstrate how their main results can be reproduced by a simple qualitative analysis of the respective magnetohydrodynamic (MHD) equations.
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Geomagnetism and Paleomagnetism Studies
