The dynamical response of the solar corona to surface and sub-surface perturbations depends on the chromospheric stratification, and specifically on how efficiently these layers reflect or transmit incoming Alfvén waves. While it would be desirable to include the chromospheric layers in the numerical simulations used to study such phenomena, that is most often not feasible. We defined and tested a simple approximation allowing the study of coronal phenomena while taking into account a parametrised chromospheric reflectivity. We addressed the problems of the transmission of the surface rotation to the corona and that of the generation of polar plumes by Alfvén waves [1, 2]. We found that a high (yet partial) effective chromospheric reflectivity is required to properly describe the angular momentum balance in the corona and the way the surface differential rotation is transmitted upwards. Alfvén wave-driven polar plumes maintain their properties for a wide range of values for the reflectivity, but they become bursty (and eventually disrupt) when the limit of total reflection is attained.

Coupling the solar surface and the corona: Coronal rotation, Alfvén wave-driven polar plumes / R. F. Pinto;R. Grappin;M. Velli;A. Verdini. - In: AIP CONFERENCE PROCEEDINGS. - ISSN 0094-243X. - STAMPA. - 1539:(2013), pp. 58-61. (Intervento presentato al convegno SOLAR WIND 13: Proceedings of the Thirteenth International Solar Wind Conference.) [10.1063/1.4810989].

Coupling the solar surface and the corona: Coronal rotation, Alfvén wave-driven polar plumes

VELLI, MARCO;VERDINI, ANDREA
2013

Abstract

The dynamical response of the solar corona to surface and sub-surface perturbations depends on the chromospheric stratification, and specifically on how efficiently these layers reflect or transmit incoming Alfvén waves. While it would be desirable to include the chromospheric layers in the numerical simulations used to study such phenomena, that is most often not feasible. We defined and tested a simple approximation allowing the study of coronal phenomena while taking into account a parametrised chromospheric reflectivity. We addressed the problems of the transmission of the surface rotation to the corona and that of the generation of polar plumes by Alfvén waves [1, 2]. We found that a high (yet partial) effective chromospheric reflectivity is required to properly describe the angular momentum balance in the corona and the way the surface differential rotation is transmitted upwards. Alfvén wave-driven polar plumes maintain their properties for a wide range of values for the reflectivity, but they become bursty (and eventually disrupt) when the limit of total reflection is attained.
2013
SOLAR WIND 13: Proceedings of the Thirteenth International Solar Wind Conference.
SOLAR WIND 13: Proceedings of the Thirteenth International Solar Wind Conference.
R. F. Pinto;R. Grappin;M. Velli;A. Verdini
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/865913
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