The influence of the medium physical conditions and atomic constants on the Stokes profiles of absorption lines in the solar spectrum

Physics

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Scientific paper

In the frame of Unno-Beckers-Landy degl'Innocenti theory the estimations of the magnetic strengthening of the FeI lines are obtained and their behavior depending on the excitation potential, the wavelength, the equivalent width, the Lande factor, the microturbulent velocity, the bulk velocity, the damping constant, the atmospheric model, the strength and direction of the magnetic field is studied. Variations of the Stokes profiles presented in the graphic form allow the initial values of input parameters to be obtained when deriving the magnetic field vector by the inversion code. The obtained dependences of magnetic strengthening allow the correct choice of magnetic sensitive lines to be realized when simulation of the structure inhomogeneity.

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