most citedIon Scale Electromagnetic Waves in the Inner Heliosphere

128 citations · 217 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202127 cited

Small-scale Magnetic Flux Ropes with Field-aligned Flows via the PSP In-situ Observations

Yu Chen, Qiang Hu, Lingling Zhao +2

Magnetic flux rope, formed by the helical magnetic field lines, can sometimes remain its shape while carrying significant plasma flow that is aligned with the local magnetic field.…

astro-ph.SR2021

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…

astro-ph.SR2021

Solar wind energy flux observations in the inner heliosphere: First results from Parker Solar Probe

M. Liu, K. Issautier, N. Meyer-Vernet +15

We investigate the solar wind energy flux in the inner heliosphere using 12-day observations around each perihelion of Encounter One (E01), Two (E02), Four (E04), and Five (E05) of…

physics.space-ph201914 cited

Kinetic Scale Spectral Features of Cross Helicity and Residual Energy in the Inner Heliosphere

Daniel Vech, Justin C. Kasper, Kristopher G. Klein +17

In this Paper, we present the first results from the Flux Angle operation mode of the Faraday Cup instrument onboard Parker Solar Probe. The Flux Angle mode allows rapid measuremen…

astro-ph.SR201948 cited

The Enhancement of Proton Stochastic Heating in the near-Sun Solar Wind

Mihailo M. Martinović, Kristopher G. Klein, Justin C. Kasper +18

Stochastic heating is a non-linear heating mechanism driven by the violation of magnetic moment invariance due to large-amplitude turbulent fluctuations producing diffusion of ions…

astro-ph.SR2019128 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…