activity
20192021
most citedMagnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounter

161 citations · 264 across the 5 of their papers we have counts for

collaborators

10 papers

physics.plasm-ph2021

Nonlinear Interactions in Spherically Polarized Alfvénic Turbulence

Trevor A. Bowen, Samuel T. Badman, Stuart D. Bale +8

Turbulent magnetic field fluctuations observed in the solar wind often maintain a constant magnitude condition accompanied by spherically polarized velocity fluctuations; these sig…

astro-ph.SR2021

Plasma Properties, Switchback Patches and Low -Particle Abundance in Slow Alfvénic Coronal Hole Wind at 0.13 au

Thomas Woolley, Lorenzo Matteini, Michael D. McManus +8

The Parker Solar Probe (PSP) mission presents a unique opportunity to study the near-Sun solar wind closer than any previous spacecraft. During its fourth and fifth solar encounter…

physics.space-ph2021

Using Parker Solar Probe observations during the first four perihelia to constrain global magnetohydrodynamic models

Pete Riley, Roberto Lionello, Ronald M. Caplan +4

Parker Solar Probe (PSP) is providing an unprecedented view of the Sun's corona as it progressively dips closer into the solar atmosphere with each solar encounter. Each set of obs…

astro-ph.SR2021

The active region source of a type III radio storm observed by Parker Solar Probe during Encounter 2

L. Harra, D. H. Brooks, S. D. Bale +6

Context. To investigate the source of a type III radio burst storm during encounter 2 of NASA's Parker Solar Probe (PSP) mission. Aims. It was observed that in encounter 2 of NASA'…

physics.space-ph2020

Statistical analysis of orientation, shape, and size of solar wind switchbacks

Ronan Laker, Timothy S. Horbury, Stuart D. Bale +9

One of the main discoveries from the first two orbits of Parker Solar Probe (PSP) was the presence of magnetic switchbacks, whose deflections dominated the magnetic field measureme…

astro-ph.SR2020

Switchbacks as signatures of magnetic flux ropes generated by interchange reconnection in the corona

J. F. Drake, O. Agapitov, M. Swisdak +10

The structure of magnetic flux ropes injected into the solar wind during reconnection in the coronal atmosphere is explored with particle-in-cell simulations and compared with in s…