activity
20082017
most citedKink instabilities in jets from rotating magnetic fields

95 citations · 520 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2017★ 59 cited

Double-diffusive erosion of the core of Jupiter

R. Moll, P. Garaud, C. Mankovich +1

We present Direct Numerical Simulations of the transport of heat and heavy elements across a double-diffusive interface or a double-diffusive staircase, in conditions that are clos…

astro-ph.SR2016★ 29 cited

The effect of rotation on oscillatory double-diffusive convection (semiconvection)

Ryan Moll, Pascale Garaud

Oscillatory double-diffusive convection (ODDC, more traditionally called semiconvection) is a form of linear double-diffusive instability that occurs in fluids that are unstably st…

physics.plasm-ph2015★ 29 cited

Plasma Viscosity with Mass Transport in Spherical ICF Implosion Simulations

Erik L. Vold, Archis S. Joglekar, Mario I. Ortega +3

The effects of viscosity and small-scale atomic-level mixing on plasmas in inertial confinement fusion (ICF) currently represent challenges in ICF research. Many current ICF hydrod…

astro-ph.SR2015★ 33 cited

A New Model for Mixing By Double-Diffusive Convection (Semi-Convection). III. Thermal and Compositional Transport Through Non-Layered ODDC

Ryan Moll, Pascale Garaud, Stephan Stellmach

Oscillatory double-diffusive convection (ODDC) (also known as semi- convection) refers to a type of double diffusive instability that occurs in regions of planetary and stellar int…

astro-ph.HE2012★ 26 cited

Shearing box simulations of accretion disk winds

R. Moll

The launching process of a magnetically driven outflow from an accretion disk is investigated in a local, shearing box model which allows a study of the feedback between accretion…

astro-ph.SR2012★ 84 cited

Vortices, shocks, and heating in the solar photosphere: effect of a magnetic field

R. Moll, R. H. Cameron, M. Schüssler

Aims: We study the differences between non-magnetic and magnetic regions in the flow and thermal structure of the upper solar photosphere. Methods: Radiative MHD simulations repres…