Flattening of the Density Spectrum in Compressible Hall-MHD Simulations

Flattening of the Density Spectrum in Compressible Hall-MHD Simulations

Observations of proton density fluctuations of the solar wind at 1 au have shown the presence of a decade-long transition region of the density spectrum above sub-ion scales, characterized by a flattening of the spectral slope. We use the proton density fluctuations data collected by the BMSW instru...

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Bibliographic Details
Main Authors: Victor Montagud-Camps, František Němec, Jana Šafránková, Zdeněk Němeček, Andrea Verdini, Roland Grappin, Emanuele Papini, Luca Franci
Format: Article
Language:English
Published: MDPI AG 2021-09-01
Series:Atmosphere
Subjects:
plasma turbulence
density spectrum
solar wind
Online Access:https://www.mdpi.com/2073-4433/12/9/1162

Internet

https://www.mdpi.com/2073-4433/12/9/1162

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