Schrinner, M.; Schmitt, D.; Cameron, R.; Hoyng, P.: Saturation and time dependence of geodynamo models. Geophysical Journal International 182, pp. 675 - 681 (2010)
Schrinner, M.; Schmitt, D.; Jiang, J.; Hoyng, P.: An efficient method for computing the eigenfunctions of the dynamo equation. Astronomy and Astrophysics 519, A80 (2010)
Jiang, J.; Cameron, R.; Schmitt, D.; Schüssler, M.: Countercell Meridional Flow and Latitudinal Distribution of the Solar Polar Magnetic Field. Astrophysical Journal 693, pp. L96 - L99 (2009)
Solanki, S. K.; Wenzler, T.; Schmitt, D.: Moments of the latitudinal dependence of the sunspot cycle: A new diagnostic of dynamo models. Astronomy and Astrophysics 483, pp. 623 - 632 (2008)
Holzwarth, V.; Schüssler, M.; Schmitt, D.: Flow instabilities of magnetic flux tubes - II. Longitudinal flow. Astronomy and Astrophysics 469, pp. 11 - 17 (2007)
Işık, E.; Schmitt, D.; Schüssler, M.: A coupled model of magnetic flux generation and transport in stars. Astron. Nachrichten 328, pp. 1111 - 1113 (2007)
Schrinner, M.; Rädler, K.-H.; Schmitt, D.; Rheinhardt, M.; Christensen, U. R.: Mean-field concept and direct numerical simulations of rotating magnetoconvection and the geodynamo. Geophys. Astrophys. Fluid Dynamics 101, pp. 81 - 116 (2007)
Baumann, I.; Schmitt, D.; Schüssler, M.: A necessary extension of the surface flux transport model. Astronomy and Astrophysics 446, pp. 307 - 314 (2006)
Baumann, I.; Schmitt, D.; Schüssler, M.: A necessary extension of the flux transport model. Memorie della Societa Astronomica Italiana 76, pp. 933 - 936 (2005)
Schrinner, M.; Rädler, K.-H.; Schmitt, D.; Rheinhardt, M.; Christensen, U.: Mean-field view on rotating magnetoconvection and a geodynamo model. Astron. Nachrichten 326, pp. 245 - 249 (2005)
Baumann, I.; Schmitt, D.; Schüssler, M.; Solanki, S. K.: Evolution of the large-scale magnetic field on the solar surface: a parameter study. Astronomy and Astrophysics 426, pp. 1075 - 1091 (2004)
Kolesnikov, F.; Bünte, M.; Schmitt, D.; Schüssler, M.: Kelvin-Helmholtz and shear instability of a helical flow around a magnetic flux tube. Astronomy and Astrophysics 420 (2), pp. 737 - 749 (2004)
Hoyng, P.; Schmitt, D.; Ossendrijver, M. A. J. H.: A theoretical analysis of the observed variability of the geomagnetic dipole field. Physics of the Earth and Planetary Interiors 130, pp. 143 - 157 (2002)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.