Hydrodynamic modeling of tomographically reconstructed coronal loops

The solar corona is structured by the magnetic field in the form of loops or flux tubes. During periods of minimum solar activity or in the quiescent corona (outside active regions), density and temperature inhomogeneities between loops and their surroundings are relatively low, making them not easi...

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Detalles Bibliográficos
Autores principales:	Mac Cormack, C., López Fuentes, M., Mandrini, Cristina Hemilse, Lloveras, D. G., Vásquez, A. M.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2021
Materias:	Ciencias Astronómicas Sun: corona Sun: magnetic fields Sun: UV radiation
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/165203
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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