RECENT OBSERVATIONAL AND THEORETICAL WORK ON SOLAR WIND TURBULENCE AND DISSIPATION SUGGESTS THAT KINETIC-SCALE FLUCTUATIONS ARE BOTH HEATING AND ISOTROPIZING THE SOLAR WIND DURING TRANSIT TO 1 AU. THE NATURE OF THESE FLUCTUATIONS AND ASSOCIATED HEATI
$520,337FY2020National Aeronautics and Space AdministrationNASA
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