activity
20052016
most citedMean-field concept and direct numerical simulations of rotating magnetoconvection and the geodynamo

231 citations · 1.1k across the 24 of their papers we have counts for

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6 papers · 1 filter

astro-ph.EP2014★ 11 cited

Hemispherical Parker waves driven by thermal shear in planetary dynamos

Wieland Dietrich, Dieter Schmitt, Johannes Wicht

Planetary and stellar magnetic fields are thought to be sustained by helical motions (-effect) and, if present, differential rotation (-effect). In the Sun, the strong differ…

astro-ph.EP2011★ 3 cited

A domino model for geomagnetic field reversals

N. Mori, D. Schmitt, A. Ferriz-Mas +4

We solve the equations of motion of a one-dimensional planar Heisenberg (or Vaks-Larkin) model consisting of a system of interacting macro-spins aligned along a ring. Each spin has…

astro-ph.EP2011★ 11 cited

Coupled spin models for magnetic variation of planets and stars

A. Nakamichi, H. Mouri, D. Schmitt +3

Geomagnetism is characterized by intermittent polarity reversals and rapid fluctuations. We have recently proposed a coupled macro-spin model to describe these dynamics based on th…

astro-ph.EP2011★ 3 cited

Mode analysis of numerical geodynamo models

Martin Schrinner, Dieter Schmitt, Peter Hoyng

It has been suggested in Hoyng (2009) that dynamo action can be analysed by expansion of the magnetic field into dynamo modes and statistical evaluation of the mode coefficients. W…

astro-ph.EP2010★ 14 cited

The initial temporal evolution of a feedback dynamo for Mercury

D. Heyner, D. Schmitt, J. Wicht +3

Various possibilities are currently under discussion to explain the observed weakness of the intrinsic magnetic field of planet Mercury. One of the possible dynamo scenarios is a d…

astro-ph.EP2009★ 21 cited

Saturation and time dependence of geodynamo models

M. Schrinner, D. Schmitt, R. Cameron +1

In this study we address the question under which conditions a saturated velocity field stemming from geodynamo simulations leads to an exponential growth of the magnetic field in…