A Statistical Study of the Compressible Energy Cascade Rate in Solar Wind Turbulence: Parker Solar Probe Observations
Maia Brodiano, Pablo Dmitruk, Nahuel Andr\'es

TL;DR
This study analyzes the energy cascade rates in solar wind turbulence at various distances from the Sun using Parker Solar Probe data, revealing increased cascade rates closer to the Sun and with higher plasma compressibility.
Contribution
It applies two recent exact relations for compressible MHD turbulence to observational data, providing new insights into how cascade rates vary with heliocentric distance and plasma compressibility.
Findings
Cascade rates increase closer to the Sun.
Compressibility correlates with higher cascade rates.
Similar cascade rates are observed regardless of the exact relation used.
Abstract
We investigated incompressible and compressible magnetohydrodynamic (MHD) energy cascade rates in the solar wind at different heliocentric distances. We used in situ magnetic field and plasma observations provided by the Parker Solar Probe (PSP) mission and exact relations in fully developed turbulence. To estimate the compressible cascade rate, we applied two recent exact relations for compressible isothermal and polytropic MHD turbulence, respectively. Our observational results show a clear increase of the absolute value of the compressible and incompressible cascade rates as we get closer to the Sun. Moreover, we obtained an increase in both isothermal and polytropic cascade rates with respect to the incompressible case as compressibility increases in the plasma. Further discussion about the relation between the compressibility and the heliocentric distance is carried out.…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics · Solar Radiation and Photovoltaics
