Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment

A central problem of space plasma physics is how protons and electrons are heated in a turbulent, magnetized plasma. The differential heating of charged species due to dissipation of turbulent fluctuations plays a key role in solar wind evolution. Measurements from previous heliophysics missions hav...

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Bibliographic Details

Published in:	The Astrophysical Journal Letters
Main Authors:	R. Bandyopadhyay, C. M. Meyer, W. H. Matthaeus, D. J. McComas, S. R. Cranmer, J. S. Halekas, J. Huang, D. E. Larson, R. Livi, A. Rahmati, P. L. Whittlesey, M. L. Stevens, J. C. Kasper, S. D. Bale
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Subjects:	Solar wind Interplanetary physics Interplanetary turbulence Solar coronal heating Magnetohydrodynamics
Online Access:	https://doi.org/10.3847/2041-8213/acf85e