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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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

id	todo:paper_17439213_v7_nS286_p437_LunaCardozo
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spelling	todo:paper_17439213_v7_nS286_p437_LunaCardozo2023-10-03T16:31:43Z Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations Luna-Cardozo, M. Verth, G. Erdélyi, R. Mandrini C.H. Webb D.F. (magnetohydrodynamics:) MHD Sun: corona Sun: fundamental parameters Sun: magnetic fields Sun: oscillations Waves 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 observations. Here, MHD wave theory is further developed illustrating how information about the magnetic and density structure along coronal loops can be determined by measuring the frequencies of the slow MHD oscillations. The application to observations of slow magnetoacoustic waves in coronal loops is discussed. © 2012 International Astronomical Union. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p437_LunaCardozo
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-134
collection	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic	(magnetohydrodynamics:) MHD Sun: corona Sun: fundamental parameters Sun: magnetic fields Sun: oscillations Waves
spellingShingle	(magnetohydrodynamics:) MHD Sun: corona Sun: fundamental parameters Sun: magnetic fields Sun: oscillations Waves Luna-Cardozo, M. Verth, G. Erdélyi, R. Mandrini C.H. Webb D.F. Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
topic_facet	(magnetohydrodynamics:) MHD Sun: corona Sun: fundamental parameters Sun: magnetic fields Sun: oscillations Waves
description	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 observations. Here, MHD wave theory is further developed illustrating how information about the magnetic and density structure along coronal loops can be determined by measuring the frequencies of the slow MHD oscillations. The application to observations of slow magnetoacoustic waves in coronal loops is discussed. © 2012 International Astronomical Union.
format	SER
author	Luna-Cardozo, M. Verth, G. Erdélyi, R. Mandrini C.H. Webb D.F.
author_facet	Luna-Cardozo, M. Verth, G. Erdélyi, R. Mandrini C.H. Webb D.F.
author_sort	Luna-Cardozo, M.
title	Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
title_short	Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
title_full	Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
title_fullStr	Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
title_full_unstemmed	Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
title_sort	magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
url	http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p437_LunaCardozo
work_keys_str_mv	AT lunacardozom magnetoseismologyofsolaratmosphericloopsbymeansoflongitudinaloscillations AT verthg magnetoseismologyofsolaratmosphericloopsbymeansoflongitudinaloscillations AT erdelyir magnetoseismologyofsolaratmosphericloopsbymeansoflongitudinaloscillations AT mandrinich magnetoseismologyofsolaratmosphericloopsbymeansoflongitudinaloscillations AT webbdf magnetoseismologyofsolaratmosphericloopsbymeansoflongitudinaloscillations
_version_	1807319190738042880

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

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