Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4960
Title: Wave propagation in the magnetic network on the Sun
Authors: Hasan, S. S
Vigeesh, G
van Ballegooijen, A. A
Keywords: Sun: Magnetic Fields - Magnetohydrodynamics (MHD);Sun: Photosphere - Oscillations
Issue Date: 2006
Publisher: Cambridge University Press
Citation: Volker Bothmer; Ahmed Abdel Hady. eds., Solar Activity and its Magnetic Origin, Proceedings of the 233rd Symposium of the International Astronomical Union held in Cairo, Egypt, March 31 - April 4, 2006, pp. 116 - 117
Series/Report no.: International Astronomical Union Symposium; No. 233
Abstract: Hasan et al. (2005) have recently presented 2-D dynamical calculations on wave propagation in in the magnetic network of the Sun. The latter is idealized as consisting of non-potential flux tubes in the quiet solar chromosphere. It is of interest to understand how the nature of wave propagation is influenced by the choice of initial equilibrium configuration of the magnetic field. We examine this by comparing the earlier calculations with those when the network is modelled as a potential structure. Our calculations demonstrate that the nature of the wave propagation is significantly different, particularly the transport of energy which for the potential case, occurs more isotropically than for the non-potential configuration.
Description: Restricted Access
URI: http://hdl.handle.net/2248/4960
ISBN: 0-521-86342-0
???metadata.dc.relation.uri???: http://dx.doi.org/10.1017/S174392130600161X
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Wave Propagation in the Magnetic Network of the SunRestricted Access374.81 kBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.