About the author
Peter Riley
Dr. Riley studies the large scale structure of the solar corona and inner heliosphere as well as the eruption and evolution of coronal mass ejections, and their interactions with the solar wind. He uses global magnetohydrodynamic (MHD) models to interpret coronal and heliospheric observations in an effort to understand the underlying physical processes at work.
Post by Peter Riley
By Ron Caplan, Jon Linker, Cooper Downs, Tibor Török, Zoran Mikić, Roberto Lionello, Viacheslav Titov, Peter Riley and Janvier Wijaya |