Heating of coronal active regions

Recent observations of coronal loops in solar active regions show that their heating must be a truly dynamic process. Even though it seems clear that the energy source is the magnetic field that confines the coronal plasma, the details of how it dissipates are still a matter of debate. In this prese...

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Guardado en:
Detalles Bibliográficos
Autor principal: Gomez, Daniel Osvaldo
Publicado: 2010
Materias:
Magnetic fiels
MHD
Sun: corona
Sun: X-rays
Turbulence
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v6_nS273_p44_Gomez
http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS273_p44_Gomez
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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