activity
20022017
most citedCarbon Ignition in Type Ia Supernovae: II. A Three-Dimensional Numerical Model

112 citations · 482 across the 11 of their papers we have counts for

collaborators

11 papers

physics.flu-dyn2017★ 5 cited

Validity of Sound-Proof Approaches in Rapidly-Rotating Compressible Convection: Marginal Stability vs. Turbulence

Jan Verhoeven, Gary A. Glatzmaier

The validity of the anelastic approximation has recently been questioned in the regime of rapidly-rotating compressible convection in low Prandtl number fluids (Calkins et al. 2015…

astro-ph2008★ 62 cited

Differential rotation in giant planets maintained by density-stratified turbulent convection

Gary A. Glatzmaier, Martha Evonuk, Tamara M. Rogers

The zonal winds on the surfaces of giant planets vary with latitude. Jupiter and Saturn, for example, have several bands of alternating eastward (prograde) and westward (retrograde…

astro-ph2008★ 44 cited

Nonlinear Dynamics of Gravity Wave Driven Flows in the Solar Radiative Interior

T. M. Rogers, K. B. MacGregor, G. A. Glatzmaier

We present results of nonlinear numerical simulations of gravity wave driven shear flow oscillations in the equatorial plane of the solar radiative interior. These results show tha…

astro-ph2008★ 25 cited

A note on "Constraints on deep-seated zonal winds inside Jupiter and Saturn"

Gary A. Glatzmaier

Liu et al. 2008 discuss an important consideration for models of zonal winds deep within giant planets. However, the constraints they propose for the depth of the winds are based o…

astro-ph2008★ 2 cited

Evolution of progenitor stars of Type Ibc supernovae and long gamma-ray bursts

S. -C. Yoon, N. Langer, M. Cantiello +2

We discuss how rotation and binary interactions may be related to the diversity of type Ibc supernovae and long gamma-ray bursts. After presenting recent evolutionary models of mas…

astro-ph2006★ 17 cited

The Effects of Rotation Rate on Deep Convection in Giant Planets with Small Solid Cores

Martha Evonuk, Gary A. Glatzmaier

We study how the pattern of thermal convection and differential rotation in the interior of a giant gaseous planet is affected by the presence of a small solid core as a function o…