MAGNETIC CYCLES IN GLOBAL LARGE-EDDY SIMULATIONS OF SOLAR CONVECTION

By M. Ghizaru, Paul Charbonneau, Piotr K. Smolarkiewicz. 2010

220 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/841138841ad62eccde2035c762fc6c36e9aa173b

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Paul Charbonneau
2. I. Usoskin
3. Mark S. Miesch
4. J. Toomre
5. M. Browning
6. A. Brun
7. S. Solanki
8. G. Kovaltsov

In Molecular Biology

1. Paul Charbonneau
2. Mark S. Miesch
3. I. Usoskin
4. J. Toomre
5. M. Browning
6. A. Brun
7. Benjamin P. Brown
8. M. Lockwood

Citations in the corpus

• MAGNETIC WREATHS AND CYCLES IN CONVECTIVE DYNAMOS (2012, background): “Recent work by Ghizaru et al. (2010) has shown large-scale organization of the toroidal field as well as magnetic activity cycles in a solar-like simulation; regular reversals of global magnetic polarity with a roughly 60 year period for a complete cycle were achieved.”
• CYCLIC MAGNETIC ACTIVITY DUE TO TURBULENT CONVECTION IN SPHERICAL WEDGE GEOMETRY (2012, methodology): “Later, oscillatory solutions have been obtained from similar simulations with subgrid-scale modeling (Ghizaru et al. 2010; Racine et al. 2011).”
• The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets (2015, background): “Although modern solar-type dynamo models reproduce the “regular” part of the behaviour of the large-scale solar magnetic field (Ghizaru et al. 2010; Brown et al. 2011; Schrinner et al. 2012; Gastine et al. 2012; Käpylä et al. 2012), it is still challenging to extend the integration time over several…”
• Solar Dynamo Theory (2014, methodology): “…again organizes itself in a longitudinal stack of elongated rolls with their axes parallel to the rotation axis (see Figure 2a) (cf. Käpylä et al. 2010, their figure 2; Brown et al. 2011, their figure 3a,b; Ghizaru et al. 2010, their figure 1; and Miesch & Toomre 2009, their section 2.2.3).”
• MAGNETIC CYCLES IN A CONVECTIVE DYNAMO SIMULATION OF A YOUNG SOLAR-TYPE STAR (2011, background): “Recent results by (Ghizaru et al. 2010) achieve both large-scale organization and cyclic reversals of polarity in a convection simulation with an underlying tachocline.”