Geodesic
Modelling of explosive magnetorotational phenomena: from~2D to~3D
Buletinul Academiei de Ştiinţe a Republicii Moldova. Matematica, no. 3 (2007), pp. 55-63.

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In the paper we describe the results of mathematical modelling of magnetorotational(MR) supernova explosion in 1D and 2D approach and formulate the problems and features for the numerical approach to simulations of the MR supernovae in 3D case. 
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     title = {Modelling of explosive magnetorotational phenomena: {from~2D} {to~3D}},
     journal = {Buletinul Academiei de \c{S}tiin\c{t}e a Republicii Moldova. Matematica},
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G. S. Bisnovatyi-Kogan; S. G. Moiseenko; B. P. Rybakin; G. V. Secrieru. Modelling of explosive magnetorotational phenomena: from~2D to~3D. Buletinul Academiei de Ştiinţe a Republicii Moldova. Matematica, no. 3 (2007), pp. 55-63. http://geodesic.mathdoc.fr/item/BASM_2007_3_a4/

[1] Aftersmoth M. J., Berger M. J., Melton J. E., J. AIAA, 1998, no. 36(6), 952

[2] Ardeljan N. V., Bisnovatyi-Kogan G. S., Kosmachevskii K. V., Moiseenko S. G., Astrophysics, 47:1 (2004) | DOI

[3] Ardeljan N. V., Bisnovatyi-Kogan G. S., Moiseenko S. G., MNRAS, 359 (2005), 333 | DOI

[4] Ardelyan N. V., Bisnovatyi-Kogan G. S., Popov Yu. P., Astron. Zh., 56 (1979), 1244

[5] Ardelyan N. V., Bisnovatyi-Kogan G. S., Popov Yu. P., Chernigovsky S. V., Astron. Zh., 64 (1987), 761

[6] Ardeljan N. V., Kosmachevskii K. V., Comput. Math. Modelling, 6 (1995), 209 | DOI | MR

[7] Balsara D. S., Norton G. D., Parallel Computing, 27 (2001), 37 | DOI | Zbl

[8] Berger M., Rigoutsos I., IEEE Trans. System Man Cybernetics, 21 (1991), 61 | DOI

[9] Bisnovatyi-Kogan G. S., Astron. Zh., 47 (1970), 813

[10] Bisnovatyi-Kogan G. S., Stellar Physics, 2 volumes, Springer, 2001

[11] Bisnovatyi-Kogan G. S., Popov Yu. P., Samochin A. A., Astrophys. and Space Sci., 41 (1976), 321 | DOI | Zbl

[12] Buras R., Rampp M., Janka H. Th., Kifonidis K., Phys. Rev. Lett., 90 (2003), 241101 | DOI

[13] Gingold R. A., Monaghan J. J., MNRAS, 181 (1977), 375 | Zbl

[14] Kulikovsky A. G., Pogorelov N. V., Semenov A. Yu., Mathematical problems of the numerical solution of sets of hyperbolic equations, FIZMATLIT, Moskva, 2001

[15] Leblanc L. M., Wilson J. R., ApJ, 161 (1970), 541 | DOI

[16] Lucy L. B., ApJ, 82 (1977), 1013

[17] Moiseenko S. G., Bisnovatyi-Kogan G. S., Ardeljan N. V., MNRAS, 370 (2006), 501

[18] Pushkina I. G., Tishkin V. F., Mathematical modeling, 12:3 (2000), 97–109 | MR | Zbl