Abstract Details

Name: SAMRAT SEN
Affiliation: Indian Institute of Astrophysics
Conference ID: ASI2016_541
Title : Model of a flux tube with twisted magnetic fields
Authors and Co-Authors : A. Mangalam, Indian Institute of Astrophysics
Abstract Type : Poster
Abstract Category : Sun and the Solar System
Abstract : We assume a single open magnetic flux tube spanning the solar photosphere and the lower corona in magnetohydrostatic equilibrium within a realistic stratified atmosphere subject to solar gravity. We explore variants of the self-similar sunspot model with twisted magnetic fields. The analytical solution of the variation of magnetic field strength with the depth is used to derive the run of plasma density and pressure. The aim is to apply this model as the background condition for numerical studies of energy transport mechanisms from the solar surface to the corona taking realistic inputs of field strength and pressure distribution observed in the lower solar atmosphere.