Abstract
A discontinuity cannot exist in astrophysical plasma with magnetic field if small perturbations disintegrate it into other discontinuities or transform it to a more general non-steady flow. In this chapter we consider the so-called evolutionarity or structural stability of the classic discontinuous solution of the MHD equations.
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Somov, B.V. (2013). Evolutionarity of MHD Discontinuities. In: Plasma Astrophysics, Part I. Astrophysics and Space Science Library, vol 391. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-4283-7_17
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