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The Nature of Turbulence at Subelectron Scales in the Solar Wind

  • Authors: Shiladittya Mondal, Christopher H. K. Chen, Davide Manzini

Shiladittya Mondal et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

Power spectral density of (a) Vsc and (b) B (MAG—grey, SCM—blue). The least-squares fits (vertically shifted for clarity) and the break frequency (fb) using Equation (1) are shown by the black dashed lines and the diamond marker, respectively. Thin grey dashed lines indicate the flat analog-to-digital converter and the frequency dependent SCM noise floors. (c) Vsc and B spectra compensated by the sub-ion range scaling ﹩({f}^{-{\alpha }_{1}}P(f))﹩. The compensated spectra shown are faded for SNR ≲2.

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