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20152023
most citedThe Solar Probe Cup on Parker Solar Probe

218 citations · 1.4k across the 25 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2023

The Effects of Non-Equilibrium Velocity Distributions on Alfvén Ion-Cyclotron Waves in the Solar Wind

Jada Walters, Kristopher G. Klein, Emily Lichko +3

In this work, we investigate how the complex structure found in solar wind proton velocity distribution functions (VDFs), rather than the commonly assumed two-component bi-Maxwelli…

astro-ph.SR2023

Ion-Driven Instabilities in the Inner Heliosphere II: Classification and Multi-Dimensional Mapping

Mihailo M. Martinovic, Kristopher G. Klein

Linear theory is a well developed framework for characterizing instabilities in weakly collisional plasmas, such as the solar wind. In the previous instalment of this series, we an…

astro-ph.SR2023

Quantifying the Energy Budget in the Solar Wind from 13.3-100 Solar Radii

J. S. Halekas, S. D. Bale, M. Berthomier +10

A variety of energy sources, ranging from dynamic processes like magnetic reconnection and waves to quasi-steady terms like the plasma pressure, may contribute to the acceleration…

astro-ph.SR2021

How Alfvén waves energize the solar wind: heat vs work

Jean C. Perez, Benjamin D. G. Chandran, Kristopher G. Klein +1

A growing body of evidence suggests that the solar wind is powered to a large extent by an Alfvén-wave (AW) energy flux. AWs energize the solar wind via two mechanisms: heating and…

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.SR202161 cited

Inferred Linear Stability of Parker Solar Probe Observations using One- and Two-Component Proton Distributions

K. G. Klein, J. L. Verniero, B. Alterman +12

The hot and diffuse nature of the Sun's extended atmosphere allows it to persist in non-equilibrium states for long enough that wave-particle instabilities can arise and modify the…