ONE OF THE MAJOR CHALLENGES IN HELIOPHYSICS IS THE CHARACTERIZATION OF THE GLOBAL STRUCTURE AND EVOLUTION OF CORONAL MASS EJECTIONS (CMES) AFTER THEY ERUPT FROM THE SUN. CURRENTLY THE MAGNETIC CONFIGURATION OF CMES IS EITHER INFERRED INDIRECTLY FROM
$461,717FY2022National Aeronautics and Space AdministrationNASA
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