Magnetic field and plasma scaling laws: Their implications for coronal heating models

In order to test different models of coronal heating, we have investigated how the magnetic field strength of coronal flux tubes depends on the end-to-end length of the tube. Using photospheric magnetograms from both observed and idealized active regions, we computed potential, linear force-free, an...

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Autores principales: Mandrini, C.H., Démoulin, P., Klimchuk, J.A.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v530_n2PART1_p999_Mandrini
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