Gradient tensor invariants serve as proxies for mechanistic energy fluxes and bound available flux in MHD turbulence, with exact expressions for hydrodynamic cases.
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Simulations show MUSE-resolution intensity spectra can infer the density fluctuation spectrum inside coronal loops.
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A tensor invariant approach to energy flux in magnetohydrodynamic turbulence
Gradient tensor invariants serve as proxies for mechanistic energy fluxes and bound available flux in MHD turbulence, with exact expressions for hydrodynamic cases.
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Numerical simulations of waves and turbulence in coronal loops: observables and spectra
Simulations show MUSE-resolution intensity spectra can infer the density fluctuation spectrum inside coronal loops.