Preferential Proton over Electron heating from coherent structures during the first perihelion of Parker Solar Probe

Abstract

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 magnetic coherent structures identified by means of the Partial Variance of Increments (PVI) method. Statistically, regions of space with strong gradients in the magnetic field, $PVI\ge 1$, are associated with strongly enhanced proton but only slightly elevated electron temperatures. Our analysis indicates a heating mechanism in the nascent solar wind environment facilitated by a nonlinear turbulent cascade that preferentially heats protons over electrons.

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Cited by in corpus (2)

• Proton and electron temperatures in the solar wind and their correlations with the solar wind speed
• Evolution of MHD turbulence in the expanding solar wind: residual energy and intermittency