Turbulence Causality-Constrained PANS Model for MHD Simulation of the Solar Wind
Dr. Rohit Chhiber, BSc (Honours), MSc, PhD1, Arcadi V. Usmanov2, Prof. William H Matthaeus2, Arakel Petrosyan3, Tulasi Parashar2, Yan Yang2 and Melvyn L Goldstein4, (1)University of Delaware, Department of Physics and Astronomy, Newark, United States, (2)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (3)Space Research Institute RAS, Moscow, Russia, (4)Space Science Institute Boulder, Boulder, United States
