Abstract
We consider first the procedures used to measure properties of the 3D spectra and then of 1D spectra.
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Reference
Verdini A, Grappin R (2016) Beyond the maltese cross: geometry of turbulence between 0.2 and 1 Au. Astrophys J 831(2):1–8
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Montagud-Camps, V. (2019). Defining Spectral Properties in EBM Simulations. In: Turbulent Heating and Anisotropy in the Solar Wind. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-30383-9_6
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DOI: https://doi.org/10.1007/978-3-030-30383-9_6
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