WE USE REMOTE SENSING OBSERVATIONS SPANNING MULTIPLE REGIMES TO CHARACTERIZE THE NATURE OF EMISSION IN THE MIDDLE CORONA (1.3 3 RSUN) AND DERIVE THE CONDITIONS PROCESSES AND MAGNETIC CONNECTIVITY THAT GIVE RISE TO TRANSIENT AND STEADY OUTFLOWS THAT
$523,307FY2022National Aeronautics and Space AdministrationNASA
Southwest Research Institute, San Antonio TX