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Dependence of Coronal Loop Temperature on Loop Length and Magnetic Field Strength
Dahlburg, R.~B.; Einaudi, G.; Ugarte-Urra, I.; Rappazzo, A.~F.; Velli, M.;
Published by: \apj Published on: 12/2018
YEAR: 2018   DOI: 10.3847/1538-4357/aae535
Parker Data Used; magnetohydrodynamics: MHD; Sun: activity; Sun: corona; turbulence