Radial Evolution and Energy Budget of Thermal and Suprathermal Electron Populations in the Slow Solar Wind from 0.13 to 0.5 AU : Parker Solar Probe observations.
Joel Baby Abraham1, Christopher John Owen2, Daniel Verscharen3, Robert T Wicks4, Georgios Nicolaou5, Jefferson Agudelo Rueda6, Seong-Yeop Jeong7, David Stansby8, Mayur Bakrania9, Laura Bercic9 and Phyllis L Whittlesey10, (1)University College London, London, United Kingdom, (2)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, (3)University of New Hampshire Main Campus, Durham, NH, United States, (4)Northumbria University, Newcastle-Upon-Tyne, United Kingdom, (5)UTSA, Rymdcampus, San Antonio, TX, United States, (6)Dartmouth College, Physics and Astronomy, Hanover, United States, (7)Northumbria University, Mathematics, Physics and Electrical Engineering, Newcastle-Upon-Tyne, United Kingdom, (8)Imperial College London, London, SW7, United Kingdom, (9)Mullard Space Science Laboratory, University College London, London, United Kingdom, (10)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States
