Babcock, H. W. (1961), The topology of the sun's magnetic field and the 22-year cycle, Astrophys.~J., 133, 572, doi:10.1086/147060. [CrossRef]
Busse, F. H. (2002), Convective flows in rapidly rotating spheres and their dynamo action, Phys. Fluids, 14, 1301, doi:10.1063/1.1455626. [CrossRef]
Busse, F. H. (2004), On thermal convection in slowly rotating systems, Chaos, 14, 803, doi:10.1063/1.1774413. [CrossRef]
Busse, F. H., E. Grote, and A. Tilgner (1998), On convection driven dynamos in rotating spherical shells, Stud. Geophys. Geod., 42, 211, doi:10.1023/A:1023370314270. [CrossRef]
Dobler, W., and A. V. Getling (2004), Compressible magnetoconvection as the local producer of solar-type magnetic structures, in: Multi-Wavelength Investigations of Solar Activity, Proc. IAU Symp. 223, St. Petersburg, Russia, 2004, edited by A. V. Stepanov, E. E. Benevolenskaya, and A. G. Kosovichev, p. 239, Cambridge Univ. Press, New York.
Getling, A. V. (1998), Rayleigh-Bénard Convection: Structures and Dynamics, World Sci., Singapore.
Getling, A. V. (2001), Convective mechanism for the formation of photospheric magnetic fields, Astron. Rep. (in Engl. transl.), 45, 569.
Getling, A. V., and I. L. Ovchinnikov (2002), Solar convection as the producer of magnetic bipoles, in: The 10th European Solar Physics Meeting "Solar Variability: From Core to Outer Frontiers", SP 506, p. 819, Eur. Space Agency Spec. Publ., Prague.
Getling, A. V., and B. A. Tverskoy (1971a), A model of the oscillatory hydromagnetic dynamo: I, Geomagn. Aeron. (in Russian), 11, 211.
Getling, A. V., and B. A. Tverskoy (1971b), A model of the oscillatory hydromagnetic dynamo: II, Geomagn. Aeron. (in Russian), 11, 389.
Grote, E., F. H. Busse, and A. Tilgner (1999), Convection-driven quadrupolar dynamos in rotating spherical shells, Phys. Rev. E, 60, R5025, doi:10.1103/PhysRevE.60.R5025. [CrossRef]
Grote, E., F. H. Busse, and A. Tilgner (2000), Regular and chaotic spherical dynamos, Phys. Earth Planet. Inter., 117, 259, doi:10.1016/S0031-9201(99)00101-6. [CrossRef]
Krause, F., and K.-H. Rädler (1980), Mean-Field Electrodynamics and Dynamo Theory, Akademie, Berlin, Germany.
Leighton, R. B. (1964), Transport of magnetic fields on the Sun, Astrophys.~J., 140, 1547, doi:10.1086/148058. [CrossRef]
Leighton, R. B. (1969), A magneto-kinematic model of the solar cycle, Astrophys.~J., 156, 1, doi:10.1086/149943. [CrossRef]
Moffatt, H. K. (1978), Magnetic Field Generation in Electrically Conducting Fluids, Cambridge Univ. Press, New York.
Schrijver, C. J., and C. Zwaan (2000), Solar and Stellar Magnetic Activity, Cambridge Univ. Press, New York.
Simitev, R., and F. H. Busse (2002), Parameter dependences in convection driven spherical dynamos, in: High Performance Computing in Science and Engineering'02, edited by E. Krause and W. Jäger, p. 15, Springer, New York.
Simitev, R., and F. H. Busse (2005), Prandtl number dependence of convection driven dynamos in rotating spherical fluid shells, J. Fluid Mech., 532, 365, doi:10.1017/S0022112005004398. [CrossRef]
Tilgner, A. (1999), Spectral methods for the simulation of incompressible flows in spherical shells, Int. J. Numer. Methods Fluids, 30, 713, doi:10.1002/(SICI)1097-0363(19990730)30:6<713::AID-FLD859>3.0.CO;2-Y. [CrossRef]
Tilgner, A., and F. H. Busse (1997), Finite-amplitude convection in rotating spherical fluid shells, J. Fluid Mech., 332, 359.
Tverskoy, B. A. (1966), Anent the theory of hydrodynamic self-excitation of regular magnetic fields, Geomagn. Aeron. (in Russian), 6, 11.