158 citations · 688 across the 26 of their papers we have counts for
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The radial variation of the solar wind turbulence spectra near the kinetic break scale from Parker Solar Probe measurements
S. Lotz, A. E. Nel, R. T. Wicks +7
In this study we examine the radial dependence of the inertial and dissipation range indices, as well as the spectral break separating the inertial and dissipation range in power d…
Interchange reconnection as the source of the fast solar wind within coronal holes
S. D. Bale, J. F. Drake, M. D. McManus +13
The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called coronal holes. The energy source responsible for acceler…
The Radial Evolution of the Solar Wind as Organized by Electron Distribution Parameters
J. S. Halekas, P. Whittlesey, D. E. Larson +9
We utilize observations from the Parker Solar Probe (PSP) to study the radial evolution of the solar wind in the inner heliosphere. We analyze electron velocity distribution functi…
Association of intermittency with electron heating in the near-Sun solar wind
C. Phillips, R. Bandyopadhyay, D. J. McComas +1
Several studies in the near-Earth environment show that intermittent structures are important sites of energy dissipation and particle energization. Recent Parker Solar Probe (PSP)…
Structure and fluctuations of a slow ICME sheath observed at 0.5 au by the Parker Solar Probe
E. K. J. Kilpua, S. W. Good, M. Ala-Lahti +5
Sheaths ahead of interplanetary coronal mass ejections (ICMEs) are turbulent heliospheric structures. Knowledge of their structure and fluctuations is important for understanding t…
Core Electron Heating By Triggered Ion Acoustic Waves In The Solar Wind
Forrest Mozer, Stuart Bale, Cynthia Cattell +4
Perihelion passes on Parker Solar Probe orbits six through nine have been studied to show that solar wind core electrons emerged from 15 solar radii with a temperature of 55 plus o…