"9"^^ . "Realistic solar prominence models combining radiative transfer modeling and MHD simulatios"@en . "9"^^ . . . . . "http://www.isvav.cz/projectDetail.do?rowId=GAP209/12/0906"^^ . "2012-01-01+01:00"^^ . "We will construct first prominence models employing sophisticated non-LTE radiative transfer modeling to obtain the synthetic radiation emerging from realistically modeled plasma of the prominence fine structures, following the 3D configuration of the magnetic field within the prominence provided by realistic MHD processes.We will also continue in further development and use of our current 2D multi-thread prominence fine-structure models with emphasis on the study of the differential emission measures of prominences and effects of the mutual radiative interaction between individual prominence fine structures. These 2D models represent a unique tool for understanding of the fundamental processes governing the interaction of the prominence plasma and the radiation field. We will also continue in analyses of the spectroscopic observations of prominences obtained by both space-born and ground-based instruments."@en . "GAP209/12/0906" . "2014-03-31+02:00"^^ . . "Realistick\u00E9 modely slune\u010Dn\u00EDch protuberanc\u00ED kombinuj\u00EDc\u00ED modelov\u00E1n\u00ED p\u0159enosu z\u00E1\u0159en\u00ED a MHD simulace" . "0"^^ . "Solar prominences radiative transfer MHD simulations"@en . . "2014-12-31+01:00"^^ . . . . . "1"^^ . . . . . "Hlavn\u00ED c\u00EDle projektu byly spln\u011Bny. Byly z\u00EDsk\u00E1ny hodnotn\u00E9 v\u00FDsledky v oblasti studia protuberanc\u00ED. Byl vyv\u00EDjen podrobn\u00FD numerick\u00FD program ur\u010Den\u00FD pro modelov\u00E1n\u00ED protuberanc\u00ED ve 3D. Program pro modelov\u00E1n\u00ED protuberanc\u00ED ve 2D byl aplikov\u00E1n na modern\u00ED data, z\u00EDskan\u00E1 zejm\u00E9na pomoc\u00ED dru\u017Eicov\u00FDch pozorov\u00E1n\u00ED. V\u00FDsledky byly publikov\u00E1ny v p\u0159edn\u00EDch astronomick\u00FDch \u010Dasopisech."@cs . . "0"^^ . "2015-05-22+02:00"^^ . . . "The main aims of the project were fulfilled. Valuable results in the field of the study of solar prominences were obtained. Detailed numerical code for the 3D prominence modelling was developed. 2D code was applied to modern data obtained mostly using satellites. The results of the project were published in prestigious journals.zasl\u00E1ny"@en . . "V r\u00E1mci navrhovan\u00E9ho projektu vyvineme prvn\u00ED modely protuberanc\u00ED vyu\u017E\u00EDvaj\u00EDc\u00ED sofistikovan\u00E9ho modelov\u00E1n\u00ED non-LTE p\u0159enosu z\u00E1\u0159en\u00ED k z\u00EDsk\u00E1n\u00ED syntetick\u00E9ho z\u00E1\u0159en\u00ED, kter\u00E9 je emitov\u00E1no realisticky popsan\u00FDm plazmatem jemn\u00E9 struktury protuberanc\u00ED. Konfigurace plazmatick\u00E9 struktury odpov\u00EDd\u00E1 3D konfiguraci magnetick\u00E9ho pole v protuberanci z\u00EDskan\u00E9 pomoc\u00ED realistick\u00FDch MHD proces\u016F. Budeme t\u00E9\u017E pokra\u010Dovat v dal\u0161\u00EDm rozvoji a vyu\u017E\u00EDv\u00E1n\u00ED st\u00E1vaj\u00EDc\u00EDch 2D mnohovl\u00E1knov\u00FDch model\u016F jemn\u00E9 struktury protuberanc\u00ED s d\u016Frazem na studium diferenci\u00E1ln\u00EDch emisn\u00EDch m\u011Br protuberanc\u00ED a efekt\u016F vz\u00E1jemn\u00E9 z\u00E1\u0159iv\u00E9 interakce jednotliv\u00FDch vl\u00E1ken jemn\u00E9 struktury protuberanc\u00ED. Tyto 2D modely p\u0159edstavuj\u00ED jedine\u010Dn\u00FD n\u00E1stroj pro na\u0161e porozum\u011Bn\u00ED fungov\u00E1n\u00ED fundament\u00E1ln\u00EDch proces\u016F ovl\u00E1daj\u00EDc\u00EDch interakci protuberan\u010Dn\u00EDho plazmatu s polem z\u00E1\u0159en\u00ED. Pokra\u010Dovat budeme taky v anal\u00FDze spektroskopick\u00FDch pozorov\u00E1n\u00ED protuberanc\u00ED z\u00EDskan\u00FDch jak z vesm\u00EDrn\u00FDch dru\u017Eic tak i z pozemn\u00EDch observato\u0159\u00ED." .