most citedAre Switchback boundaries observed by Parker Solar Probe closed?

14 citations · 22 across the 6 of their papers we have counts for

collaborators

6 papers

physics.space-ph2024★ 8 cited

Whistler waves in the young solar wind: statistics of amplitude and propagation direction from Parker Solar Probe Encounters 1-11

Kyung-Eun Choi, Oleksiy Agapitov, Lucas Colomban +5

In the interplanetary space solar wind plasma, whistler waves are observed in a wide range of heliocentric distance (from ~20 solar radii (RS) to Jupiter's orbit). They are known t…

astro-ph.SR2024

Extended Cyclotron Resonant Heating of the Turbulent Solar Wind

Trevor A. Bowen, Ivan Y. Vasko, Stuart D. Bale +8

Circularly polarized, nearly parallel propagating waves are prevalent in the solar wind at ion-kinetic scales. At these scales, the spectrum of turbulent fluctuations in the solar…

astro-ph.SR2024

The relative prevalence of wave-packets and coherent structures in the inertial and kinetic ranges of turbulence as seen by Solar Orbiter

Alina Bendt, Sandra C. Chapman, Thierry Dudok de Wit

The Solar Orbiter (SO) mission provides the opportunity to study the evolution of solar wind turbulence. We use SO observations of nine extended intervals of homogeneous turbulence…

astro-ph.SR2023★ 14 cited

Are Switchback boundaries observed by Parker Solar Probe closed?

Nina Bizien, Thierry Dudok de Wit, Clara Froment +7

Switchbacks are sudden and large deflections in the magnetic field that Parker Solar Probe frequently observes in the inner heliosphere. Their ubiquitous occurrence has prompted nu…

astro-ph.SR2023

Ion kinetics of plasma interchange reconnection in the lower solar corona

Vladimir Krasnoselskikh, Arnaud Zaslavsky, Anton Artemyev +6

The exploration of the inner heliosphere by Parker Solar Probe has revealed a highly structured solar wind with ubiquitous deflections from the Parker spiral, known as switchbacks.…

physics.space-ph2023

Mediation of Collisionless Turbulent Dissipation Through Cyclotron Resonance

Trevor A. Bowen, Stuart D. Bale, Benjamin D. G. Chandran +6

The dissipation of magnetized turbulence is fundamental to understanding energy transfer and heating in astrophysical systems. Collisionless interactions, such as resonant wave-par…