activity
20232025
most citedEstimation of turbulent proton and electron heating rates via Landau damping constrained by Parker Solar Probe observations

18 citations · 37 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20251 cited

Multi-spacecraft Measurements of the Evolving Geometry of the Solar Alfvén Surface Over Half a Solar Cycle

Samuel T. Badman, Michael L. Stevens, Stuart D. Bale +18

The geometry of a star's Alfvén surface determines stellar angular momentum loss, separates a causally distinct 'corona' and stellar wind, and potentially affects exoplanetary habi…

astro-ph.SR2025

Evidence of Interaction between Ion-Scale Waves and Ion Velocity Distributions in the Solar Wind

Yogesh, Leon Ofman, Scott A Boardsen +9

Recent in situ observations from Parker Solar Probe (PSP) near perihelia reveal ion beams, temperature anisotropies, and kinetic wave activity. These features are likely linked to…

astro-ph.SR2024

Impact of Two-Population -particle Distributions on Plasma Stability

Mihailo M. Martinović, Kristopher G. Klein, Rossana De Marco +3

The stability of weakly collisional plasmas is well represented by linear theory, and the generated waves play an essential role in the thermodynamics of these systems. The velocit…

astro-ph.SR2024

Estimated Heating Rates Due to Cyclotron Damping of Ion-scale Waves Observed by Parker Solar Probe

Niranjana Shankarappa, Kristopher Klein, Mihailo Martinovic +1

Circularly polarized waves consistent with parallel-propagating ion cyclotron waves (ICWs) and fast magnetosonic waves (FMWs) are often observed by Parker Solar Probe (PSP) at ion…

physics.space-ph2024

Higher-Order Analysis of Three-Dimensional Anisotropy in Imbalanced Alfvénic Turbulence

Nikos Sioulas, Themistocles Zikopoulos, Chen Shi +10

We analyze in-situ observations of imbalanced solar wind turbulence to evaluate MHD turbulence models grounded in "Critical Balance" (CB) and "Scale-Dependent Dynamic Alignment" (S…

astro-ph.SR202318 cited

Total Electron Temperature Derived from Quasi-Thermal Noise Spectroscopy In the Pristine Solar Wind: Parker Solar Probe Observations

M. Liu, K. Issautier, M. Moncuquet +11

The Quasi-thermal noise (QTN) technique is a reliable tool to yield accurate measurements of the electron parameters in the solar wind. We apply this method on Parker Solar Probe (…