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[1] Alven G., Feltkhammar K.-G., Kosmicheskaya elektrodinamika, Mir, M., 1967
[2] Busse F. H., “A model of the geodynamo”, Geophys. J. Roy. Asron. Soc., 42 (1975), 437–459 | Zbl
[3] Busse F. H., “Generation of planetary by convection”, Phys. Earth Planet. Inter., 12 (1976), 350–358 | DOI
[4] Zhang K.-K., Busse F. H., “Finite amplitude convection and magnetic field generation in a rotating spherical shell”, Geophys. Astrophys. Fluid Dynamics, 44 (1988), 33–54 | DOI
[5] Zhang K.-K., Busse F. H., “Convection driven magnetohydrodynamic dynamos in rotating spherical shell”, Geophys. Astrophys. Fluid Dynamics, 49 (1989), 97–116 | DOI | Zbl
[6] Zhang K.-K., Busse F. H., “Generation of magnetic fields by convection in a rotating spherical fluid shell of infinite Prandtl number”, Phys. Earth Planet. Inter., 59 (1990), 208–222 | DOI
[7] Eltayeb I. A., “Hydromagnetic convection in a rapidly rotating fluid layer”, Proc. Roy. Soc. London A, 326 (1972), 229–254 | DOI | Zbl
[8] Eltayeb I. A., “Overstable hydromagnetic convection in a rapidly rotating fluid layer”, J. Fluid Mech., 71 (1975), 161–179 | DOI | Zbl
[9] Gabov C. A., Sveshnikov A. G., Lineinye zadachi nestatsionarnykh vnutrennikh voln, Nauka, M., 1990