Authors: Chen Shi (Department of Physics, Auburn University) The solar wind is highly turbulent, containing fluctuations that span a wide range of spatial and temporalView More
Authors: Chen Shi (UCLA), Marco Velli (UCLA), Gabor Toth (University of Michigan Ann Arbor), Kun Zhang (UCLA), Anna Tenerani (UT Austin), Zesen Huang (UCLA), NikosView More
Authors: Chen Shi (UCLA), Nikos Sioulas (UCLA), Zesen Huang (UCLA), Marco Velli (UCLA), Anna Tenerani (UT Austin) We carry out 3D magnetohydrodynamic (MHD) simulations ofView More