Diagnostics of Polar Field Reversal in Solar Cycle 23 Using a Flux Transport Dynamo Model

By M. Dikpati, G. de Toma, P. Gilman, Charles N. Arge, O. White. 2004

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Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/369b913c3e2777329384b5a50b9998f68e6ed14f

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Citations in the corpus

Dynamo Models of the Solar Cycle (2005, background): “This situation carries over to the other types of models to be discussed in Sections 4.5 and 4.8, unless additional modelling assumptions are introduced (e.g., enhanced surface magnetic diffusivity, see Dikpati et al., 2004).”
Toroidal versus poloidal magnetic fields in Sun-like stars: a rotation threshold (2008, background): “…(FL); jmorin@ast.obs-mip.fr (JM); fpaletou@ast.obs-mip.fr (FP); jramirez@mesiog.obspm.fr (JR); Claude.Catala@obspm.fr (CC); rim.fares@ast.obs-mip.fr (RF) active regions by meridional circulation (Dikpati et al. 2004) as possible processes to regenerate the poloidal magnetic component.”
Solar Differential Rotation Influenced by Latitudinal Entropy Variations in the Tachocline (2006, background): “Charbonneau & Dikpati (2000) introduced random stochastic fluctuations, while Dikpati et al. (2004) and Bonnanno et al. (2005) considered multiple cells in latitude.”
Solar activity forecast with a dynamo model (2007, methodology): “We found a decaying solution, in contrast to the oscillatory solution which Dikpati et al. (2004) reported.”
Structure and Evolution of Giant Cells in Global Models of Solar Convection (2007, background): “…currently lies beyond the reach of helioseismic probing but many have proposed that an equatorward return flow may exist and furthermore that this global circulation pattern may play an essential role in establishing the solar activity cycle (Dikpati & Charbonneau 1999; Dikpati et al. 2004, e.g.).”
Predicting the strength of solar cycle 24 using a flux‐transport dynamo‐based tool (2006, methodology): “Here we propose and test a new method, based on a flux transport dynamo model that has already been demonstrated to reproduce many solar cycle features [Dikpati et al., 2004].”
Simulating and Predicting Solar Cycles Using a Flux-Transport Dynamo (2006, background): “Over the past few years, it has also been well demonstrated that meridional circulation controls the Sun’s memory about its past magnetic fields (see Dikpati et al. 2004, hereafter DDGAW04).”
Flux-Transport Dynamos with Lorentz Force Feedback on Differential Rotation and Meridional Flow: Saturation Mechanism and Torsional Oscillations (2006, background): “…dynamos have proven to be successful for modeling the evolution of the large scale solar magnetic field (Wang & Sheeley 1991; Durney 1995; Choudhuri et al. 1995; Dikpati & Charbonneau 1999; Küker et al. 2001; Dikpati & Gilman 2001; Dikpati et al. 2004; Dikpati 2005; Dikpati et al. 2006).”