292 citations · 4.2k across the 48 of their papers we have counts for
49 papers
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…
Nonlinear dynamics of small-scale Alfvén waves
Alfred Mallet, Seth Dorfman, Mel Abler +2
We study the nonlinear evolution of very oblique small-scale Alfvén waves with . At these scales, the waves become significantly compressive, unlike in MHD, d…
The effect of variations in magnetic field direction from turbulence on kinetic-scale instabilities
Simon Opie, Daniel Verscharen, Christopher H. K. Chen +2
At kinetic scales in the solar wind, instabilities transfer energy from particles to fluctuations in the electromagnetic fields while restoring plasma conditions towards thermodyna…
Conditions for proton temperature anisotropy to drive instabilities in the solar wind
Simon Opie, Daniel Verscharen, Christopher H. K. Chen +2
Using high-resolution data from Solar Orbiter, we investigate the plasma conditions necessary for the proton temperature anisotropy driven mirror-mode and oblique firehose instabil…
Applicability of Taylor's Hypothesis during Parker Solar Probe perihelia
Jean C. Perez, Sofiane Bourouaine, Christopher H. K. Chen +1
We investigate the validity of Taylor's Hypothesis (TH) in the analysis of Alfvénic fluctuations of velocity and magnetic fields in solar wind streams measured by Parker Solar Prob…
Multiscale Solar Wind Turbulence Properties inside and near Switchbacks measured by Parker Solar Probe
Mihailo M. Martinović, Kristopher G. Klein, Jia Huang +9
Parker Solar Probe (PSP) routinely observes magnetic field deflections in the solar wind at distances less than 0.3 au from the Sun. These deflections are related to structures com…