Geodesic
Traveling contrast structures in various hydromagnetic dynamo models
Matematičeskoe modelirovanie, Tome 14 (2002) no. 10, pp. 95-104

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Two models are analysed describing the propagation of the large-scale magnetic fields in galaxies. The specific patterns are considered known as magnetic fronts. The speed of the front has been derived in the principal asymptotic term. 
@article{MM_2002_14_10_a9,
     author = {A. P. Petrov},
     title = {Traveling contrast structures in various hydromagnetic dynamo models},
     journal = {Matemati\v{c}eskoe modelirovanie},
     pages = {95--104},
     publisher = {mathdoc},
     volume = {14},
     number = {10},
     year = {2002},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/MM_2002_14_10_a9/}
}
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A. P. Petrov. Traveling contrast structures in various hydromagnetic dynamo models. Matematičeskoe modelirovanie, Tome 14 (2002) no. 10, pp. 95-104. http://geodesic.mathdoc.fr/item/MM_2002_14_10_a9/