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Two-dimensional MHD models of solar magnetogranulation. Dynamics of magnetic elements
V. A. Sheminova
We present the results of a statistical analysis of the Doppler shifts and the asymmetry parameters of V profiles of the Fe I 630.25 nm line produced by 2D MHD simulations of solar…
Absolute shifts of Fe I and Fe II lines in solar active regions (disk center)
P. N. Brandt, A. S. Gadun, V. A. Sheminova
We estimated absolute shifts of Fe I and Fe II lines from Fourier-transform spectra observed in solar active regions. Weak Fe I lines and all Fe II lines tend to be red-shifted as…
Convective shifts of iron lines in the spectrum of the solar photosphere
V. A. Sheminova, A. S. Gadun
The influence of the convective structure of the solar photosphere on the shifts of spectral lines of iron was studied. Line profiles in the visible and infrared spectrum were synt…
Fourier analysis of Fe I lines in the spectra of the Sun, α Centauri A, Procyon, Arcturus, and Canopus
V. A. Sheminova, A. S. Gadun
We used spectral observations of Fe I line profiles with a 200 000 resolution to determine micro and macroturbulent velocities in the atmospheres of the Sun as a star, α Cen A, Pro…