M. I. Stodilka
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Research Interests
M. I. Stodilka has a total of 7 co-authors. Here are the top co-authors by number of shared publications:
- A. I. Prysiazhnyi
Astronomical Observatory, Ivan Franko National University of Lviv, 79005, Lviv, Ukraine
2 shared publications - Roman I. Kostik
Main Astronomical Observatory, National Academy of Sciences of Ukraine, Kyiv, Ukraine
2 shared publications - Andrii Prysiazhnyi
Ivan Franko Natl Univ Lviv, Astron Observ, 8 Kyrylo & Mefodiy St, UA-79005 Lvov, Ukraine
1 shared publication M. B. Hirnyak
Ivan Franko Natl Univ Lviv, Astron Observ, 8 Kyryla & Mefodia St, UA-79005 Lvov, Ukraine
1 shared publicationM. M. Koval'Chuk
Ivan Franko Natl Univ Lviv, Astron Observ, 8 Kyryla & Mefodia St, UA-79005 Lvov, Ukraine
1 shared publication- Oleksandra Baran
Ivan Franko Natl Univ Lviv, Astron Observ, 8 Kyrylo & Mefodiy St, UA-79005 Lvov, Ukraine
1 shared publication
Latest Publications
- 1 July 2020
- Published by Allerton Press in Kinematics and Physics of Celestial Bodies
- Vol. 36 (4) , 153-160
Solar Faculae: Microturbulence as an Indicator of Inclined Magnetic Fields
The observations of the solar facula in the Ba II λ 455.403 Å line are used to construct a 3D model of the facula area by solving the invers
- 1 July 2020
- Published by Allerton Press in Kinematics and Physics of Celestial Bodies
- Vol. 36 (4) , 153-160
Solar Faculae: Microturbulence as an Indicator of Inclined Magnetic Fields
The observations of the solar facula in the Ba II λ 455.403 Å line are used to construct a 3D model of the facula area by solving the invers
- 1 November 2019
- Published by Allerton Press in Kinematics and Physics of Celestial Bodies
- Vol. 35 (6) , 261-270
Features of Convection in the Atmospheric Layers of the Solar Facula
According to the data of complex 2D observations on the VTT telescope of the solar facula, a 3D model of the solar atmosphere in the facular region was obt
- 1 November 2019
- Published by Allerton Press in Kinematics and Physics of Celestial Bodies
- Vol. 35 (6) , 261-270
Features of Convection in the Atmospheric Layers of the Solar Facula
According to the data of complex 2D observations on the VTT telescope of the solar facula, a 3D model of the solar atmosphere in the facular region was obt
- 1 September 2019
- Published by Allerton Press in Kinematics and Physics of Celestial Bodies
- Vol. 35 (5) , 231-251
Diagnostics of the Quiet Sun Atmosphere’s Photospheric Jets
—From 2D-spectral observation data of a quiet region of the solar disk center in the Fe I λ 557.609 nm line, 3D hydrodynamic models of photospheric jets are built by solving the inverse...
- 1 September 2019
- Published by Allerton Press in Kinematics and Physics of Celestial Bodies
- Vol. 35 (5) , 231-251
Diagnostics of the Quiet Sun Atmosphere’s Photospheric Jets
—From 2D-spectral observation data of a quiet region of the solar disk center in the Fe I λ 557.609 nm line, 3D hydrodynamic models of photospheric jets are built by solving the inverse...
- 1 January 2019
- Published by Ivan Franko National University of Lviv in Journal of Physical Studies
- Vol. 23 (1)
Dynamics of the fine structure of the 22-year solar activity magnetic cycle
- 1 January 2019
- Published by Ivan Franko National University of Lviv in Journal of Physical Studies
- Vol. 23 (1)
Dynamics of the fine structure of the 22-year solar activity magnetic cycle