Subproton-scale Intermittency in Near-Sun Solar Wind Turbulence Observed by the Parker Solar Probe

TL;DR

This study analyzes solar wind turbulence near the Sun using high-resolution data from the Parker Solar Probe, revealing a transition from multifractal to monofractal intermittency at subproton scales, clarifying turbulence behavior.

Contribution

It provides the first detailed characterization of intermittency scaling from inertial to subproton scales in near-Sun solar wind, highlighting a transition to monofractality.

Findings

Multifractal scaling in the inertial range.

Monofractal, non-Gaussian scaling in subproton range.

Transition likely due to scale-invariant current sheets.

Abstract

High time-resolution solar wind magnetic field data is employed to study statistics describing intermittency near the first perihelion (~35.6 Rs) of the Parker Solar Probe mission. A merged dataset employing two instruments on the FIELDS suite enables broadband estimation of higher order moments of magnetic field increments, with five orders established with reliable accuracy. The duration, cadence, and low noise level of the data permit evaluation of scale dependence of the observed intermittency from the inertial range to deep subproton scales. The results support multifractal scaling in the inertial range, and monofractal but non-Gaussian scaling in the subproton range, thus clarifying suggestions based on data near Earth that had remained ambiguous due to possible interference of the terrestrial foreshock. The physics of the transition to monofractality remains unclear but we suggest that it is due to a scale-invariant population of current sheets between ion and electron inertial scales; the previous suggestion of incoherent kinetic-scale wave activity is disfavored as it presumably leads to re-Gaussianization which is not observed.