| 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, L Spina, G Carraro, R Gratton, ... Astronomy & Astrophysics 653, A67, 2021 | 47 | 2021 |
| On the average optical depth of formation of weak Fraunhofer lines E Gurtovenko, V Ratnikova, C De Jager Solar Physics 37, 43-52, 1974 | 41 | 1974 |
| A formation mechanism of magnetic elements in regions of mixed polarity AS Gadun, SK Solanki, VA Sheminova, SRO Ploner Solar Physics 203, 1-7, 2001 | 35 | 2001 |
| The wings of Ca II H and K as solar fluxtube diagnostics VA Sheminova, RJ Rutten Astronomy & Astrophysics 437 (3), 1069-1080, 2005 | 31 | 2005 |
| Turbulence and rotation in solar-type stars VA Sheminova Kinematics and Physics of Celestial Bodies 35 (3), 129-142, 2019 | 22 | 2019 |
| The Wings of Ca ii H and K as Photospheric Diagnostics and the Reliability of One-Dimensional Photosphere Modeling VA Sheminova Solar Physics 280, 83-102, 2012 | 18 | 2012 |
| Numerical simulation of the interaction between solar granules and small-scale magnetic fields IN Atroshchenko, VA Sheminova arXiv preprint arXiv:1011.1778, 2010 | 16* | 2010 |
| SPANSAT: the program for LTE calculations of absorption line profiles in stellar atmospheres AS Gadun, VA Sheminova Preprint of the Institute for Theoretical Physics of Academy of Sciences of …, 1988 | 16 | 1988 |
| The formation of one-lobed Stokes V profiles in an inhomogeneous atmosphere SRO Ploner, M Schussler, SK Solanki, VA Sheminova, AS Gadun, ... Advanced Solar Polarimetry--Theory, Observation, and Instrumentation 236 …, 2001 | 15 | 2001 |
| Is the FIP effect present inside solar photospheric magnetic flux tubes? VA Sheminova, SK Solanki Astronomy and Astrophysics, v. 351, p. 701-706 (1999) 351, 701-706, 1999 | 14 | 1999 |
| Fourier analysis of Fe I lines in the spectra of the Sun,{\alpha} Centauri A, Procyon, Arcturus, and Canopus VA Sheminova, AS Gadun arXiv preprint arXiv:1004.3286, 2010 | 12 | 2010 |
| Sensitivity indicators of Fraunhofer lines VA Sheminova Astronomy and Astrophysics, v. 329, p. 721-724 (1998) 329, 721-724, 1998 | 12 | 1998 |
| ‘Crossing’ method for studying the turbulence in solar and stellar atmospheres: I: Application to the Sun EA Gurtovenko, VA Sheminova Solar physics 106, 237-247, 1986 | 12 | 1986 |
| What is the difference between ‘emission’and ‘depression’contribution functions? EA Gurtovenko, VA Sheminova, AP Sarychev Solar physics 136, 239-250, 1991 | 11 | 1991 |
| Parameters of sensitivity of Fraunhofer lines to changes in the temperature, gas pressure, and microturbulent velocity in the solar photosphere VA Sheminova arXiv preprint arXiv:1210.5375, 2012 | 10 | 2012 |
| Evolution of solar magnetic tubes from observations of Stokes parameters VA Sheminova, AS Gadun Astronomy Reports 44, 701-710, 2000 | 10 | 2000 |
| Kinematika i Fizika Nebes AS Gadun, VA Sheminova, SK Solanki Tel [Kinematics and Physics of Celestial Bodies] 15 (5), 387-397, 1999 | 10 | 1999 |
| Absolute shifts of Fe I and Fe II lines in solar active regions (disk center) PN Brandt, AS Gadun, VA Sheminova arXiv preprint arXiv:1005.2064, 2010 | 8 | 2010 |
| On the origin of the extremely asymmetric Stokes V profiles in an inhomogeneous atmosphere VA Sheminova Kinematika i Fizika Nebesnykh Tel 21 (3), 172-196, 2005 | 8 | 2005 |
| Calculating the Profiles of Stokes Parameters of Magnetoactive Absorption Lines in Stellar Atmospheres VA Sheminova Kiev (VINITI File No. 2940-V90, 30 May 1990), 1990 | 7 | 1990 |
Luc Rouppe van der VoortUniversity of Oslo在 astro.uio.no 的电子邮件经过验证
Luc Rouppe van der VoortUniversity of Oslo在 astro.uio.no 的电子邮件经过验证