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NASA NTRS · 19910041659

Does ion tearing exist?

Abstract

Theoretical models of reconnection in the geomagnetic tail and its relationship to the collisionless tearing mode are examined analytically. The focus is on attempts to remove the stabilizing effects of electron compressibility in the quasi-neutral sheet. It is shown that this goal can be achieved by introducing spatial diffusion of electrons across the magnetic-flux surfaces, but not by wave-turbulent pitch-angle scattering (Coroniti, 1980) or nonadiabatic stochastic first-invariant diffusion (Buechner and Zelenyi, 1988). Hence the ion tearing mode does not exist, but the electron tearing mode does.

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BibTeXRIS

Pellat, R., Coroniti, F. V., Pritchett, P. L.. 1991-02-01. Does ion tearing exist?. https://ntrs.nasa.gov/citations/19910041659

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