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Three-dimensional Stokes inversion with magnetohydrostationary constraints

Subject Area Astrophysics and Astronomy
Term from 2016 to 2020
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 321818926
 
Final Report Year 2021

Final Report Abstract

We have developed the first inversion code for the polarized radiative transfer equation capable of inferring the real three-dimensional topology (x, y, z) of the physical parameters in the atmosphere of the Sun in a way that is consistent with both Maxwell’s equations and the magneto-hydrostatic equations. The code can be employed to calculate accurate electric currents in the solar atmosphere, thereby opening the possibility of detecting non-potential configurations of the magnetic field before energetic and explosive events, that can affect the interplanetary medium and the higher layers of Earth’s atmosphere, occur.

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