A Data-constrained Analysis for Joule Heating as a Solar Active Region Atmosphere Heating Mechanism. I. Sunspot Umbral Light Bridge

Understanding the mechanisms underlying the heating of the solar atmosphere is a fundamental problem in solar physics. The lower atmosphere of the Sun (i.e., photosphere and chromosphere) is composed of weakly ionized plasma. This results in anisotropic dissipation of electric currents by Coulomb an...

Täydet tiedot

Bibliografiset tiedot

Päätekijät:	M. S. Yalim, M. Frisse, C. Beck, D. P. Choudhary, A. Prasad, S. S. Nayak, G. P. Zank
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2024-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Solar chromosphere Solar chromospheric heating Solar active region magnetic fields
Linkit:	https://doi.org/10.3847/1538-4357/ad5e75
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