Characterizing thermal expansion profile of solar wind streams with Parker Solar Probe SWEAP and FIELDS
Characterizing thermal expansion profile of solar wind streams with Parker Solar Probe SWEAP and FIELDS
Gregory Mark Szypko1, Kristoff Paulson2, Anthony W Case3, Michael Louis Stevens4, Kelly E Korreck5, Justin Christophe Kasper6, Stuart D Bale7, Christopher Mark Bert8, Phyllis L Whittlesey9, Davin E Larson10, Roberto Livi9, Keith Goetz11, John W Bonnell7, Thierry Dudok de Wit12, Peter Harvey13, Robert J MacDowall14, David Malaspina15, Marc Pulupa7 and Tatiana Niembro Hernandez16, (1)Dartmouth College, Hanover, NH, United States, (2)Smithsonian Astrophysical Observatory, Cambridge, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)Smithsonian Astrophysics Observatory, Cambridge, MA, United States, (5)Smithsonian Observatory, Cambridge, MA, United States, (6)University of Michigan, Ann Arbor, MI, United States, (7)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (8)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (9)University of California Berkeley, Berkeley, CA, United States, (10)Space Sciences Laboratory, Berkeley, CA, United States, (11)University of Minnesota, Minneapolis, MN, United States, (12)LPC2E, CNRS and University of Orléans, Orléans, France, (13)Space Sciences Laboratory, Berkeley, United States, (14)NASA/Goddard Space Flight Center, Greenbelt, United States, (15)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (16)UNAM National Autonomous University of Mexico, Fac. de Ciencias, Mexico City, Mexico
