R. Toedte

TURBULENT MAGNETIC FIELD AMPLIFICATION FROM SPIRAL SASI MODES: IMPLICATIONS FOR CORE-COLLAPSE SUPERNOVAE AND PROTO-NEUTRON STAR MAGNETIZATION

E. Endeve, C. Cardall, R. Budiardja, 2012, 1203.3108.

TURBULENT MAGNETIC FIELD AMPLIFICATION FROM SPIRAL SASI MODES: IMPLICATIONS FOR CORE-COLLAPSE SUPERNOVAE AND PROTO-NEUTRON STAR MAGNETIZATION

E. Endeve, C. Cardall, R. Budiardja, 2012, 1203.3108.

Multi-scale data visualization for computational astrophysics and climate dynamics at Oak Ridge National Laboratory

George Ostrouchov, Jinzhu Gao, Sean Ahern, 2006 .