activity
20182022
most citedEnhanced Energy Transfer Rate in Solar Wind Turbulence Observed near the Sun from Parker Solar Probe

81 citations · 523 across the 16 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2022

Magnetic Switchback Occurrence Rates in the Inner Heliosphere: Parker Solar Probe and 1 au

Francesco Pecora, William H. Matthaeus, Leonardo Primavera +4

The subject of switchbacks, defined either as large angular deflections or polarity reversals of the magnetic field, has generated substantial interest in the space physics communi…

physics.space-ph202246 cited

Intermittency in the Expanding Solar Wind: Observations from Parker Solar Probe (0.16au), Helios 1 (0.3-1au), and Voyager 1 (1-10au)

Manuel Enrique Cuesta, Tulasi N. Parashar, Rohit Chhiber +1

We examine statistics of magnetic field vector components to explore how intermittency evolves from near sun plasma to radial distances as large as 10 au. Statistics entering the a…

physics.space-ph202267 cited

Sub-Alfvenic Solar Wind observed by PSP: Characterization of Turbulence, Anisotropy, Intermittency, and Switchback

R. Bandyopadhyay, W. H. Matthaeus, D. J. McComas +18

In the lower solar coronal regions where the magnetic field is dominant, the Alfven speed is much higher than the wind speed. In contrast, the near-Earth solar wind is strongly sup…

astro-ph.SR202227 cited

Statistical analysis of intermittency and its association with proton heating in the near Sun environment

Nikos Sioulas, Marco Velli, Rohit Chhiber +9

We use data from the first six encounters of Parker Solar Probe and employ the Partial Variance of Increments () method to study the statistical properties of coherent structu…

physics.space-ph202150 cited

Subproton-scale Intermittency in Near-Sun Solar Wind Turbulence Observed by the Parker Solar Probe

Rohit Chhiber, William H. Matthaeus, Trevor A. Bowen +1

High time-resolution solar wind magnetic field data is employed to study statistics describing intermittency near the first perihelion (~35.6 Rs) of the Parker Solar Probe mission.…

astro-ph.SR2020

Magnetic Field Line Random Walk and Solar Energetic Particle Path Lengths: Stochastic Theory and PSP/ISoIS Observation

R. Chhiber, W. H. Matthaeus, C. M. S. Cohen +21

Context:In 2020 May-June, six solar energetic ion events were observed by the Parker Solar Probe/ISoIS instrument suite at 0.35 AU from the Sun. From standard velocity-dispersion a…