Radial velocity fluctuations at Parker Solar Probe during closest approach in encounter 22
Radial velocity fluctuations at Parker Solar Probe during closest approach in encounter 22
Federico Fraschetti1, Samuel Timothy Badman2, Srijan Bharati Das3, Tatiana Niembro Hernandez4, Kristoff W Paulson5, Yeimy Rivera6, Michael Louis Stevens7, Michael Terres6, Davin Larson8, Roberto Livi9, Ali Rahmati9, Orlando Romeo10, Zesen Huang11, Marco C M Velli12, Stuart Bale13 and Sylvain Korzennik6, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)University of Oxford, Oxford, United Kingdom, (3)Princeton University, Princeton, United States, (4)UNAM National Autonomous University of Mexico, Fac. de Ciencias, Mexico City, Mexico, (5)University of New Hampshire, Chelmsford, United States, (6)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (7)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (8)University of California Berkeley, Berkeley, United States, (9)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (10)University of Maryland, College Park, College Park, United States, (11)University of Science and Technology of China, Hefei, Anhui, China, (12)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, (13)University of California, Berkeley, Berkeley, CA, United States