Abstract: Abstract The problem of the existence of self-similar solutions for astrophysical magnetohydrodynamic (MHD) transient flows is considered. Our approach is based on the pioneering works by B.C. Low for coronal transients and their further generalizations. The axiomatic basis of the approach is adjusted and verified. It is shown that the introduction of a new type of “triple-compound” variable may lead to the appearance of new classes of analytic self-similar solutions, possibly relevant for a number of interesting astrophysical situations. T...
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Topics: 
Astrophysics
Astronomy
Mechanics