activity
20172026
most citedNonlinear energy transfer and current sheet development in localized Alfven wavepacket collisions in the strong turbulence limit

25 citations · 25 across the 11 of their papers we have counts for

collaborators

11 papers

physics.plasm-ph2026

Phase-Space Energy Transfer of Wave-Particle Interactions using the Field-Particle Correlation Technique and Linear Plasma Theory with JET-PLUME

Collin R. Brown, Gregory G. Howes, Kristopher G. Klein +1

The collisionless transfer of energy between fields and particles through wave-particle interactions is a fundamental process in space plasmas but remains incompletely characterize…

physics.plasm-ph2026

Plasma Instabilities in Arbitrary Distributions: Comparison between ALPS and BO

Xudong Guo, Huasheng Xie, Kristopher G. Klein +3

Determining accurate wave dispersion relations is a central problem in plasma physics. Recent advances have enabled the numerical computation of linear dispersion relation in plasm…

astro-ph.SR2026

The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations

Hao Ran, Daniel Verscharen, Jesse Coburn +6

Observations of solar wind velocity distribution functions (VDFs) commonly reveal fine-scale structures. These features strongly influence kinetic processes such as wave damping an…

physics.plasm-ph2026

Wave-particle equilibria with heavy ions in weakly collisional space plasmas

Nicolás Villarroel-Sepúlveda, Daniel Verscharen, Pablo S. Moya +2

Space plasmas are weakly collisional since characteristic time scales related to Coulomb collisions are much larger than those of Larmor gyration or wave--particle interactions. Th…

astro-ph.SR2026

Solar Wind Heating Near the Sun: A Radial Evolution Approach

Yogesh, Leon Ofman, Kristopher Klein +19

Characterizing the plasma state in the near-Sun environment is essential to constrain the mechanisms that heat and accelerate the solar wind. In this study, we use Parker Solar Pro…

physics.plasm-ph2026

Velocity-Space Signatures of Energy Transfer for Ion-Acoustic Instabilities

Mahmoud Saad Afify, Kristopher G. Klein, Mihailo M. Martinović +1

Context. Observations by Parker Solar Probe (PSP) of electrostatic waves suggest that electrostatic instabilities, including the ion-ion-acoustic instability (IIAI) frequently obse…

astro-ph.SR2025

How the Oblique Drift Instability Alters Solar Wind Heating and Constrains the Distribution of Solar Wind Observations

Mihailo M. Martinovic, Kristopher G. Klein, Leon Ofman +6

Ion-driven plasma instability thresholds, derived from linear theory, constrain the distribution of solar observations in parameter space, defining boundaries of stable plasma para…

astro-ph.SR2025

Observational Constraints on the Radial Evolution of O Temperature and Differential Flow in the Inner Heliosphere

Yeimy J. Rivera, Kristopher G. Klein, Joseph H. Wang +15

Over decades of solar wind observations, heavy ions have been observed to have a higher temperature and flow faster than protons in the solar corona and heliosphere. Remote observa…

physics.plasm-ph2025

The Dielectric Response of Plasmas with Arbitrary Gyrotropic Velocity Distributions

Kristopher Klein, Daniel Verscharen

Hot and tenuous plasmas are frequently far from local thermodynamic equilibrium, necessitating sophisticated methods for determining the associated plasma dielectric tensor and nor…

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…

physics.plasm-ph2017★ 25 cited

Nonlinear energy transfer and current sheet development in localized Alfven wavepacket collisions in the strong turbulence limit

J. L. Verniero, G. G. Howes, K. G. Klein

In space and astrophysical plasmas, turbulence is responsible for transferring energy from large scales driven by violent events or instabilities, to smaller scales where turbulent…