MHS sunspot model from deep sub-photospheric to chromospheric layers

Details MHS sunspot model from deep sub-photospheric to chromospheric layers MHS sunspot model from deep sub-photospheric to chromospheric layers

2008-08-26

arxiv.org/abs/0808.3571v1

Astronomy and Astrophysics

Astrophysics

accepted by ApJ

Scientific paper

10.1086/592681

In order to understand the influence of magnetic fields on the propagation properties of waves, as derived from different local helioseismology techniques, forward modeling of waves is required. Such calculations need a model in magnetohydrostatic equilibrium as initial atmosphere to propagate oscillations through it. We provide a method to construct such a model in equilibrium for a wide range of parameters to be used for simulations of artificial helioseismologic data. The method combine the advantages of self-similar solutions and current-distributed models. A set of models is developed by numerical integration of magnetohydrostatic equations from the sub-photospheric to chromospheric layers.

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