Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field

The energy transfer between a homogeneous heat-conducting collisionless plasma in a strong magnetic field and a harmonic external current immersed in it is studied in connection with the generation of stable magnetohydrodynamic waves in slow streams in the solar-wind plasma. The net balance of energ...

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Autor principal: De La Torre, A.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00223778_v43_n3_p475_DeLaTorre
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spelling todo:paper_00223778_v43_n3_p475_DeLaTorre2023-10-03T14:32:32Z Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field De La Torre, A. The energy transfer between a homogeneous heat-conducting collisionless plasma in a strong magnetic field and a harmonic external current immersed in it is studied in connection with the generation of stable magnetohydrodynamic waves in slow streams in the solar-wind plasma. The net balance of energy, given by the sum of the individual contriButions that result from the interchange between each mode of oscillation and the stream, is established as function of the amplitude, frequency and growing rate of the external current and the plasma parameters. © 1990, Cambridge University Press. All rights reserved. Fil:De La Torre, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00223778_v43_n3_p475_DeLaTorre
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description The energy transfer between a homogeneous heat-conducting collisionless plasma in a strong magnetic field and a harmonic external current immersed in it is studied in connection with the generation of stable magnetohydrodynamic waves in slow streams in the solar-wind plasma. The net balance of energy, given by the sum of the individual contriButions that result from the interchange between each mode of oscillation and the stream, is established as function of the amplitude, frequency and growing rate of the external current and the plasma parameters. © 1990, Cambridge University Press. All rights reserved.
format JOUR
author De La Torre, A.
spellingShingle De La Torre, A.
Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field
author_facet De La Torre, A.
author_sort De La Torre, A.
title Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field
title_short Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field
title_full Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field
title_fullStr Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field
title_full_unstemmed Energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field
title_sort energy budget of stable magnetohydrodynamic waves in a homogeneous heat-conducting collisionless plasma in a strong magnetic field
url http://hdl.handle.net/20.500.12110/paper_00223778_v43_n3_p475_DeLaTorre
work_keys_str_mv AT delatorrea energybudgetofstablemagnetohydrodynamicwavesinahomogeneousheatconductingcollisionlessplasmainastrongmagneticfield
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