Estimating the contribution of Alfvén waves to the process of heating the quiet solar corona
作者： J. J. González-Avilés , F. S. Guzmán
DOI: 10.1093/MNRAS/STV959
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摘要: We solve numerically the ideal MHD equations with an external gravitational field in 2D order to study effects of impulsively generated linear and non-linear Alfv\'en waves into isolated solar arcades coronal funnels. analyze region containing interface between photosphere corona. The main interest is possibility that triggers energy flux transfer toward quiet corona heat it, including case two consecutive can occur. find arcades, short or large, transferred fluxes by are sufficient only during a small lapse time certain region. In funnels threshold achieved when wave faster than 10 km/s, which extremely high. conclude from our analysis, waves, even optimistic scenario having pulses, cannot transport enough as
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