On the interpretation of Parker Solar Probe Turbulent Signals

Abstract

In this letter we propose a practical methodology to interpret future Parker Solar Probe (PSP) turbulent time signals even when Taylor's hypothesis is not valid. By extending Kraichnan's sweeping model used in hydrodynamics we derive the Eulerian spacetime correlation function in magnetohydrodynamics (MHD) turbulence. It is shown that in MHD, the temporal decorrelation of small-scale fluctuations arises from a combination of hydrodynamic sweeping induced by large-scale fluid velocity $\delta u_0$ and by the Alfvénic propagation along the local magnetic field. The resulting temporal part of the space-time correlation function is used to determine the wavenumber range $\Delta k_{\perp }=[k_{\min },k_{\max }]$ of the turbulent fluctuations that contribute to the power of a given frequency $\omega$ of the time signal measured in the spacecraft frame. Our analysis also shows that the shape of frequency power spectrum $P_{sc}(\omega )$ of the time signal will follow the same power-law of the reduced power spectrum $E(k_{\perp })\sim k_{\perp }^{-\alpha }$ in the plasma frame, where $\alpha$ is the spectral index. The proposed framework for the analysis of PSP time signals entirely relies on two simple dimensionless parameters that can be empirically obtained from PSP measurements, namely, $\epsilon =\delta u_0/\sqrt{2}{V}_{\perp }$ (where $V_{\perp }$ is the perpendicular velocity of PSP seen in the plasma frame) and the spectral index $\alpha$.

5 pages, 1 figure, accepted for publication in ApJL 2019

References in corpus (4)

• Anisotropic scaling of magnetohydrodynamic turbulence
• The Violation of the Taylor Hypothesis in Measurements of Solar Wind Turbulence
• A Modified Version of Taylor's Hypothesis for Solar Probe Plus Observations
• On the spatio-temporal behavior of magnetohydrodynamic turbulence in a magnetized plasma

Cited by in corpus (9)

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• Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum
• Clustering of Intermittent Magnetic and Flow Structures near Parker Solar Probe's First Perihelion -- A Partial-Variance-of-Increments Analysis
• The Radial Dependence of Proton-scale Magnetic Spectral Break in Slow Solar Wind during PSP Encounter 2
• Turbulence characteristics of switchbacks and non-switchbacks intervals observed by \emph{Parker Solar Probe}
• The Near-Sun Streamer Belt Solar Wind: Turbulence and Solar Wind Acceleration
• Applicability of Taylor's Hypothesis during Parker Solar Probe perihelia
• The radial variation of the solar wind turbulence spectra near the kinetic break scale from Parker Solar Probe measurements
• On the Interpretation of the Scalings of Density Fluctuations from In-situ Solar Wind Observations: Insights from 3D Turbulence Simulations