activity
20192023
most citedThe Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere

270 citations · 538 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023

Observations and Modeling of Unstable Proton and Alpha Particle Velocity Distributions in Sub-Alfvenic Solar Wind at PSP Perihelia

Leon Ofman, Scott A Boardsen, Lan K Jian +7

Past observations show that solar wind (SW) acceleration occurs inside the sub-Alfvenic region, reaching the local Alfven speed at typical distances ~ 10 - 20 Rs (solar radii). Rec…

physics.space-ph2023★ 12 cited

The Temperature, Electron, and Pressure Characteristics of Switchbacks: Parker Solar Probe Observations

Jia Huang, Justin C. Kasper, Davin E. Larson +19

Parker Solar Probe (PSP) observes unexpectedly prevalent switchbacks, which are rapid magnetic field reversals that last from seconds to hours, in the inner heliosphere, posing new…

physics.space-ph2023★ 18 cited

Parker Solar Probe Observations of High Plasma Beta Solar Wind from Streamer Belt

Jia Huang, J. C. Kasper, Davin E. Larson +23

In general, slow solar wind from the streamer belt forms a high plasma beta equatorial plasma sheet around the heliospheric current sheet (HCS) crossing, namely the heliospheric pl…

physics.space-ph2023★ 25 cited

The Structure and Origin of Switchbacks: Parker Solar Probe Observations

Jia Huang, J. C. Kasper, L. A. Fisk +25

Switchbacks are rapid magnetic field reversals that last from seconds to hours. Current Parker Solar Probe (PSP) observations pose many open questions in regard to the nature of sw…

astro-ph.SR2022★ 17 cited

Density And Velocity Fluctuations of Alpha Particles in Magnetic Switchbacks

M. D. McManus, J. L. Verniero, S. D. Bale +9

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. W…

astro-ph.SR2021★ 68 cited

The In Situ Signature of Cyclotron Resonant Heating

Trevor A. Bowen, Benjmin D. G. Chandran, Jonathan Squire +9

The dissipation of magnetized turbulence is an important paradigm for describing heating and energy transfer in astrophysical environments such as the solar corona and wind; howeve…

astro-ph.SR2019★ 128 cited

Ion Scale Electromagnetic Waves in the Inner Heliosphere

Trevor Bowen, Alfred Mallet, Jia Huang +22

Understanding the physical processes in the solar wind and corona which actively contribute to heating, acceleration, and dissipation is a primary objective of NASA's Parker Solar…

astro-ph.SR2019★ 270 cited

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere

C. H. K. Chen, S. D. Bale, J. W. Bonnell +21

The first two orbits of the Parker Solar Probe (PSP) spacecraft have enabled the first in situ measurements of the solar wind down to a heliocentric distance of 0.17 au (or 36 Rs).…