Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations

There is increasingly strong observational evidence that slow magnetoacoustic modes arise in the solar atmosphere. Solar magneto-seismology is a novel tool to derive otherwise directly un-measurable properties of the solar atmosphere when magnetohydrodynamic (MHD) wave theory is compared to wave obs...

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Detalles Bibliográficos
Autores principales: Luna-Cardozo, M., Verth, G., Erdélyi, R., Mandrini C.H., Webb D.F.
Formato: SER
Materias:
(magnetohydrodynamics:) MHD
Sun: corona
Sun: fundamental parameters
Sun: magnetic fields
Sun: oscillations
Waves
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p437_LunaCardozo
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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