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physics.space-ph2026

Noise in Synthetic and Solar Wind Data: Superposition Principles

Jiaming Wang, Francesco Pecora, Rohit Chhiber +3

The interplanetary magnetic field exhibits a distinctive spectral density from frequencies of around $\unit[10^{-6}]{Hz}$ to around $\unit[10^{-4}]{Hz}$, ranging from harmoni…

physics.space-ph2025

Angular dependence of third-order law in anisotropic MHD turbulence

Bin Jiang, Zhuoran Gao, Yan Yang +6

In solar wind turbulence, the energy transfer/dissipation rate is typically estimated using MHD third-order structure functions calculated using spacecraft observations. However, t…

physics.space-ph2025

Turbulence in the terrestrial magnetosheath: space-time correlation using the Magnetospheric Multiscale mission

Francesco Pecora, William H. Matthaeus, Antonella Greco +4

Spatiotemporal correlation of magnetic field fluctuations is investigated using the Magnetospheric Multiscale mission in the terrestrial magnetosheath. The first observation of the…

physics.space-ph2024

Evaluation of scale-dependent kurtosis with HelioSwarm

Francesco Pecora, Francesco Pucci, Francesco Malara +4

Plasma turbulence involves complex, nonlinear interactions of electromagnetic fields and charged particles across multiple scales. Studying these phenomena in space plasmas, like t…

physics.space-ph2024

Anisotropy of Density Fluctuations in the Solar Wind at 1 au

Jiaming Wang, Rohit Chhiber, Sohom Roy +6

A well-known property of solar wind plasma turbulence is the observed anisotropy of the autocorrelations, or equivalently the spectra, of velocity and magnetic field fluctuations.…