43 citations · 122 across the 25 of their papers we have counts for
33 papers
Convective Line Shifts in the Spectra of Solar-Type Stars
V. A. Sheminova
The Doppler line shifts in the spectra of the Sun and stars with effective temperatures from 4800 to 6200 K were measured and the average connective (granulation) velocities were e…
The influence of the medium physical conditions and atomic constants on the Stokes profiles of absorption lines in the solar spectrum
V. A. Sheminova
The Stokes profiles of Fe I lines in the photosphere of the Sun are calculated within the Unno-Beckers-Landi-Dagl`Innocenti theory. Estimates of the magnetic strengthening of the l…
Macro-microturbulence in the solar photosphere
V. A. Sheminova
The velocity distribution of the large and small-scale motion in solar photosphere has been obtained by crossing method based on fitting the observed and calculated equivalent widt…
Influence of the vertical and horizontal magnetic field inhomogeneity on the Stokes parameters of the magnetically sensitive Fe I line 525.02 nm
V. G. Lozitskii, V. A. Sheminova
Based on calculations of the Stokes parameters for the Holweger-Mliller model atmosphere, we study sensitivity of the Fe I 525.02 nm line to some kinds of vertical and horizontal m…
Effect of the anomalous dispersion in the solar atmosphere on results of magnetic field measurements by the line-ratio method
V. G. Lozitskii, V. A. Sheminova
On the basis of Stokes parameter calculations for the Fe I 524.7 and 525.0 nm lines and the Holweger-Muller model atmosphere, the effect of the anomalous dispersion on solar magnet…
The Gaia-ESO Survey: A new approach to chemically characterising young open clusters II. Abundances of the neutron-capture elements Cu, Sr, Y, Zr, Ba, La, and Ce
M. Baratella, V. D'Orazi, V. Sheminova +32
Young open clusters (t<200 Myr) have been observed to exhibit several peculiarities in their chemical compositions, from a slightly sub-solar iron content, super-solar abundances o…