On the properties of Alfv\'enic switchbacks in the expanding solar wind: three-dimensional numerical simulations

TL;DR

This study uses 3D simulations to analyze Alfvénic switchbacks in the solar wind, predicting their properties and comparing them with Parker Solar Probe observations to understand their origin.

Contribution

The paper provides detailed 3D simulation predictions of switchback properties, highlighting effects of the Parker spiral and Alfvén waves, aiding differentiation between surface and in-situ origins.

Findings

Magnetic field deflections become asymmetric due to the Parker spiral.

Switchback magnetic field and density fluctuations depend on plasma beta.

Magnetic field and density dropouts at switchback boundaries match observations.

Abstract

Switchbacks -- abrupt reversals of the magnetic field within the solar wind -- have been ubiquitously observed by Parker Solar Probe (PSP). Their origin, whether from processes near the solar surface or within the solar wind itself, remains under debate, and likely has key implications for solar wind heating and acceleration. Here, using three-dimensional expanding box simulations, we examine the properties of switchbacks arising from the evolution of outwards-propagating Alfv\'en waves in the expanding solar wind in detail. Our goal is to provide testable predictions that can be used to differentiate between properties arising from solar surface processes and those from the in-situ evolution of Alfv\'en waves in switchback observations by PSP. We show how the inclusion of the Parker spiral causes magnetic field deflections within switchbacks to become asymmetric, preferentially deflecting in the plane of the Parker spiral and rotating in one direction towards the radial component of the mean field. The direction of the peak of the magnetic field distribution is also shown to be different from the mean field direction due to its highly skewed nature. Compressible properties of switchbacks are also explored, with magnetic-field-strength and density fluctuations being either correlated or anticorrelated depending on the value of $\beta$, agreeing with predictions from theory. We also measure dropouts in magnetic-field strength and density spikes at the boundaries of these synthetic switchbacks, both of which have been observed by PSP. The agreement of these properties with observations provide further support for the Alfv\'en wave model of switchbacks.