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2017•Astronomy and AstrophysicsOpen access

Millimeter radiation from a 3D model of the solar atmosphere

M. Loukitcheva, S. M. White, S. K. Solanki, Gregory D. Fleishman, M. Carlsson

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Abstract

Aims. We use state-of-the-art, three-dimensional non-local thermodynamic equilibrium (non-LTE) radiative magnetohydrodynamic simulations of the quiet solar atmosphere to carry out detailed tests of chromospheric magnetic field diagnostics from free-free radiation at millimeter and submillimeter wavelengths (mm/submm).

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Aims. We use state-of-the-art, three-dimensional non-local thermodynamic equilibrium (non-LTE) radiative magnetohydrodynamic simulations of the quiet solar atmosphere to carry out detailed tests of chromospheric magnetic field diagnostics from free-free radiation at millimeter and submillimeter wavelengths (mm/submm).

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Available abstract

Aims. We use state-of-the-art, three-dimensional non-local thermodynamic equilibrium (non-LTE) radiative magnetohydrodynamic simulations of the quiet solar atmosphere to carry out detailed tests of chromospheric magnetic field diagnostics from free-free radiation at millimeter and submillimeter wavelengths (mm/submm).

Key concepts: Millimeter, Atmosphere (unit), Solar atmosphere, Radiative transfer, Physics, Radiation, Magnetohydrodynamic drive, Wavelength

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