Other
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.1708k&link_type=abstract
American Astronomical Society, SPD meeting #42, #17.08; Bulletin of the American Astronomical Society, Vol. 43, 2011
Other
Scientific paper
Realistic numerical simulations of solar magnetoconvection play a key role for our understanding of the basic physical phenomena in the subsurface convective boundary layer and the atmosphere. For the accurate modeling of the turbulent processes on the Sun it is important to perform the simulations with the highest possible resolution. Our results have revealed significant changes in properties of the turbulent motions when the resolution is increased. It is particularly interesting that small-scale vortex motions in the intergranular lanes become ubiquitous and strong, and play a critical role in the large-scale organization of the solar dynamics. For the comparison with observational data it is necessary to investigate relationships between the physical and spectro-polarimetric properties in various conditions of the quiet-Sun and magnetic regions, and model the observed parameters. By using the radiative line formation code, SPINOR/STOPRO, we have calculated the Stokes profiles and other characteristics for the spectral line of the Hinode/SOT and SDO/HMI instruments, and compared the simulation results with the observational data.
Kitiashvili Irina
Kosovichev Aleksandr G.
Mansour Nagi N.
Stenflo Jan Olof
Wray Alan A.
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