The deep wind structure of the giant planets: Results from an anelastic general circulation model

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Rotating convective turbulence in Earth and planetary cores (2015, background): “Such effects are likely of relevance in gas planets (e.g., Glatzmaier et al., 2009; Kaspi et al., 2009), and may be relevant in Earth-sized terrestrial cores as well (cf. Anufriev et al., 2005; Verhoeven and Stellmach, 2014).”
Anelastic convection-driven dynamo benchmarks (2011, background): “…and so allows a much larger timestep, is therefore a popular choice for studies of solar and stellar convection zones and the interior dynamics of giant planets (e.g. Glatzmaier, 1984, 1985; Brun et al., 2004; Jones et al., 2009; Jones and Kuzanyan, 2009; Miesch et al., 2000; Kaspi et al., 2009).”
AB INITIO SIMULATIONS FOR MATERIAL PROPERTIES ALONG THE JUPITER ADIABAT (2012, methodology): “…& Glatzmaier 2010; Schubert & Soderlund 2011), basic properties, such as the observed flow patterns in the atmosphere (Heimpel et al. 2005; Vasavada & Showman 2005; Kaspi et al. 2009; Gastine & Wicht 2012), still await explanations that are consistent with planetary structure and dynamo models.”