Preferential Heating of Protons over Electrons from Coherent Structures during the First Perihelion of the Parker Solar Probe

The solar wind undergoes significant heating as it propagates away from the Sun; the exact mechanisms responsible for this heating remain unclear. Using data from the first perihelion of the Parker Solar Probe mission, we examine the properties of proton and electron heating occurring within magneti...

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Veröffentlicht in:	Astrophysical journal. Letters 2022-08, Vol.935 (2), p.L29
Hauptverfasser:	Sioulas, Nikos, Shi, Chen, Huang, Zesen, Velli, Marco
Format:	Artikel
Sprache:	eng
Schlagworte:	Electron heating Electron temperatures Electrons Heating Interplanetary turbulence Magnetic fields Magnetic properties Magnetohydrodynamics Perihelions Protons Solar coronal heating Solar probes Solar wind
Online-Zugang:	Volltext
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