Density And Velocity Fluctuations of Alpha Particles in Magnetic Switchbacks
M. D. McManus, J. L. Verniero, S. D. Bale, T. A. Bowen, D. E. Larson,, J. C. Kasper, R. Livi, L. Matteini, A. Rahmati, O. Romeo, P. L. Whittlesey,, T. Woolley

TL;DR
This study investigates density, abundance, and velocity fluctuations of alpha particles within magnetic switchbacks observed by the Parker Solar Probe, revealing complex behaviors and proposing a method to estimate the wave frame from particle data.
Contribution
It provides new insights into alpha particle dynamics in switchbacks and introduces a novel technique to determine the wave frame using particle measurements alone.
Findings
No consistent alpha abundance differences inside vs outside switchbacks.
Alpha velocities can increase, decrease, or remain unchanged within switchbacks.
The wave frame can be estimated from particle data via sphere fitting.
Abstract
Magnetic switchbacks, or sudden reversals in the magnetic field's radial direction, are one of the more striking observations of Parker Solar Probe (PSP) thus far in its mission. While their precise production mechanisms are still unknown, the two main theories are via interchange reconnection events and in-situ generation. In this work density and abundance variations of alpha particles are studied inside and outside individual switchbacks. We find no consistent compositional differences in the alpha particle abundance ratio, , inside vs outside, nor do we observe any signature when separating the switchbacks according to , the ratio of alpha-proton differential speed to the wave phase speed (speed the switchback is travelling). We argue these measurements cannot be used to rule in favour of one production mechanism over the other, due to the distance…
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