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In a plasma immersed in a sheared magnetic field of shear length L s and having a density gradient of scale length L n , finite ß (plasma pressure/magnetic pressure) results in an additional stabilizing influence over and above that due to magnetic shear. Employing a full electromagnetic treatment, these finite-ß corrections are evaluated for , where a i is the ion gyration radius and k is the wave vector perpendicular to both the direction of the density gradient and the unsheared component of the magnetic field. For the parameter ranges least stabilized by shear, the dominant finite-ß- stabilization effect occurs within the region about the rational surface where the phase velocity is larger than the Alfvén speed. As ß increases toward or (ka i m/M) 2/3 [In (ML n /m|L s |)] 4/3 this finite-ß correction must be retained, where m/M = electron mass/ion mass.
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Catto et al. (1974) studied this question.
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