A photospheric bright point model

Shelyag, Sergiy, Mathioudakis, Mihalis, Keenan, Francis and Jess, David (2010) A photospheric bright point model. Astronomy & Astrophysics, 515. A107. ISSN 0004-6361

1003.1653v1.pdf - Accepted Version

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Official URL: http://dx.doi.org/10.1051/0004-6361/200913846


Aims: A magneto-hydrostatic model is constructed with spectropolarimetric properties close to those of solar photospheric magnetic bright points.

Methods: Results of solar radiative magneto-convection simulations are used to produce the spatial structure of the vertical component of the magnetic field. The horizontal component of magnetic field is reconstructed using the self-similarity condition, while the magneto-hydrostatic equilibrium condition is applied to the standard photospheric model with the magnetic field embedded. Partial ionisation processes are found to be necessary for reconstructing the correct temperature structure of the model.

Results: The structures obtained are in good agreement with observational data. By combining the realistic structure of the magnetic field with the temperature structure of the quiet solar photosphere, the continuum formation level above the equipartition layer can be found. Preliminary results are shown of wave propagation through this magnetic structure. The observational consequences of the oscillations are examined in continuum intensity and in the Fe I 6302 Å magnetically sensitive line.

Item Type: Article
Uncontrolled Keywords: Sun: oscillations – Sun: photosphere – Sun: surface magnetism – plasmas – magnetohydrodynamics (MHD) – radiative transfer
Subjects: F300 Physics
F500 Astronomy
G100 Mathematics
Department: Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering
Depositing User: Sergiy Shelyag
Date Deposited: 23 May 2016 09:34
Last Modified: 01 Aug 2021 01:05
URI: http://nrl.northumbria.ac.uk/id/eprint/26909

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