Observing Particle Energization above the Nyquist Frequency: An Application of the Field-Particle Correlation Technique
arXiv:2204.00104 · doi:10.1063/5.0092342
Abstract
The field-particle correlation technique utilizes single-point measurements to uncover signatures of various particle energization mechanisms in turbulent space plasmas. The signature of Landau damping by electrons has been found in both simulations and observations from Earth's magnetosheath using this technique, but instrumental limitations of spacecraft sampling rates present a challenge to discovering the full extent of the presence of Landau damping in the solar wind. Theory predicts that field-particle correlations can recover velocity-space energization signatures even from data that is undersampled with respect to the characteristic frequencies at which the wave damping occurs. To test this hypothesis, we perform a high-resoluation gyrokinetic simulation of space plasma turbulence, confirm that it contains signatures of electron Landau damping, and then systematically reduce the time resolution of the data to identify the point at which the signatures become impossible to recover. We find results in support of our theoretical prediction and look for a rule of thumb that can be compared with the measurement capabilities of spacecraft missions to inform the process of applying field-particle correlations to low time resolution data.
arXiv commentSubmitted to Physics of Plasmas
References in corpus (23)
- Spectrum of magnetohydrodynamic turbulence
- A Model of Turbulence in Magnetized Plasmas: Implications for the Dissipation Range in the Solar Wind
- Astrophysical Gyrokinetics: Basic Equations and Linear Theory
- Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas
- Gyrokinetic Simulations of Solar Wind Turbulence from Ion to Electron Scales
- Evidence for Electron Landau Damping in Space Plasma Turbulence
- The Solar Probe ANalyzers -- Electrons on Parker Solar Probe
- Current Sheets and Collisionless Damping in Kinetic Plasma Turbulence
- Alfven Wave Collisions, The Fundamental Building Block of Plasma Turbulence I: Asymptotic Solution
- A Weakened Cascade Model for Turbulence in Astrophysical Plasmas
- Predicted Impacts of Proton Temperature Anisotropy on Solar Wind Turbulence
- Measuring Collisionless Damping in Heliospheric Plasmas using Field-Particle Correlations
- AstroGK: Astrophysical Gyrokinetics Code
- Diagnosing collisionless energy transfer using field-particle correlations: gyrokinetic turbulence
- Evidence of Critical Balance in Kinetic Alfven Wave Turbulence Simulations
- An Oscillating Langevin Antenna for Driving Plasma Turbulence Simulations
- Spatially Localized Particle Energization by Landau Damping in Current Sheets Produced by Strong Alfven Wave Collisions
- Diagnosing collisionless energy transfer using field-particle correlations: Alfven-Ion Cyclotron Turbulence
- The Importance of Electron Landau Damping for the Dissipation of Turbulent Energy in Terrestrial Magnetosheath Plasma
- Temporal Intermittency of Energy Dissipation in Magnetohydrodynamic Turbulence
- Collisionless energy transfer in kinetic turbulence: field-particle correlations in Fourier space
- Temporal Analysis of Dissipative Structures in Magnetohydrodynamic Turbulence
- A Field-Particle Correlation Analysis of a Perpendicular Magnetized Collisionless Shock