Autor:	Martinez-Oliveros, J. C., Donea, A. -C.
Rok vydání:	2009
Předmět:	Astrophysics - Solar and Stellar Astrophysics
Druh dokumentu:	Working Paper
DOI:	10.1111/j.1745-3933.2009.00637.x
Popis:	Dynamical changes in the solar corona have proven to be very important in inducing seismic waves into the photosphere. Different mechanisms for their generation have been proposed. In this work, we explore the magnetic field forces as plausible mechanisms to generate sunquakes as proposed by Hudson, Fisher and Welsch. We present a spatial and temporal analysis of the line-of-sight magnetic field variations induced by the seismically active 2003 October 29 and 2005 January 15 solar flares and compare these results with other supporting observations. Comment: 4 pages, 4 figures, letter, Accepted in February by MNRAS
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/0902.3856 Zobrazit plný text záznamu View this record from Arxiv