activity
20112023
most citedThe multi-scale nature of the solar wind

424 citations · 4.1k across the 75 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

physics.plasm-ph2018★ 36 cited

Stochastic proton heating by kinetic-Alfvén-wave turbulence in moderately high- plasmas

Ian W. Hoppock, Benjamin D. G. Chandran, Kristopher G. Klein +2

Stochastic heating refers to an increase in the average magnetic moment of charged particles interacting with electromagnetic fluctuations whose frequencies are smaller than the pa…

physics.space-ph2018★ 5 cited

Large-scale Control of Kinetic Dissipation in the Solar Wind

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

In this Letter we study the connection between the large-scale dynamics of the turbulence cascade and particle heating on kinetic scales. We find that the inertial range turbulence…

physics.plasm-ph2018★ 36 cited

Interplay between intermittency and dissipation in collisionless plasma turbulence

Alfred Mallet, Kristopher G. Klein, Benjamin D. G. Chandran +5

We study the damping of collisionless Alfvénic turbulence by two mechanisms: stochastic heating (whose efficiency depends on the local turbulence amplitude ) and linear Landa…

physics.space-ph2018★ 73 cited

A Majority of Solar Wind Intervals Support Ion-Driven Instabilities

K. G. Klein, B. A. Alterman, M. L. Stevens +2

We perform a statistical assessment of solar wind stability at 1 AU against ion sources of free energy using Nyquist's instability criterion. In contrast to typically employed thre…

physics.space-ph2018★ 52 cited

ALPS: The Arbitrary Linear Plasma Solver

Daniel Verscharen, Kristopher G. Klein, Benjamin D. G. Chandran +3

The Arbitrary Linear Plasma Solver (ALPS) is a parallelised numerical code that solves the dispersion relation in a hot (even relativistic) magnetised plasma with an arbitrary numb…

physics.space-ph2018★ 60 cited

Magnetic Reconnection May Control the Ion-Scale Spectral Break of Solar Wind Turbulence

Daniel Vech, Alfred Mallet, Kristopher G. Klein +1

The power spectral density of magnetic fluctuations in the solar wind exhibits several power-law-like frequency ranges with a well defined break between approximately 0.1 and 1 Hz…

physics.plasm-ph2018★ 122 cited

The statistical properties of solar wind temperature parameters near 1 AU

Lynn B. Wilson, Michael L. Stevens, Justin C. Kasper +6

We present a long-duration (10 years) statistical analysis of the temperatures, plasma betas, and temperature ratios for the electron, proton, and alpha-particle populations…