. . "2374"^^ . . "1"^^ . "0"^^ . . . "The aim of this project is the study of primary energy-release processes in solar flares based on the analysis of X-ray, radi, UV, and optical emissions of solar flares and on their modelling. Data from both present (YOHKOH, SOHO, TRACE) and new space experiments (uor hard X-ray spectrometer (HXRS) launched on board of the American MTI satellite and the HESSI project) will be analysed. These data will be compared with our radio and optical observatotions. After data analysis their modelling with already prepared or newly developed models will be made. These observed data models enable us to better understand the primary energy-release processes of solar flares. A new model of the chromospheric response to flare processes will be built. Our new concept of the hard X-ray emission of neutral beams and the model of the radio emission of the plasmoid ejection will be verified. We further plan to model the reconnection process in the bursty regime with acceleration of test particles."@en . . . "78"^^ . "Diagnostics of primary energy-release processes in solar flares and their modelling"@en . "78"^^ . "C\u00EDlem projektu je studium prim\u00E1rn\u00EDch energetick\u00FDch proces\u016F ve slune\u010Dn\u00EDch erupc\u00EDch na z\u00E1klad\u011B anal\u00FDzy rentgenov\u00E9ho, radiov\u00E9ho, UV a optick\u00E9ho z\u00E1\u0159en\u00ED slune\u010Dn\u00EDch erupc\u00ED a jejich modelov\u00E1n\u00EDm. Budou anal\u00FDzov\u00E1na data jak ze st\u00E1vaj\u00EDc\u00EDch (YOHKOH, SOHO, TRACE), tak i nov\u00FDch kosmick\u00FDch experiment\u016F: z na\u0161eho spektrometru tvrd\u00E9ho rentgenov\u00E9ho z\u00E1\u0159en\u00ED (HXRS), kter\u00FD byl vypu\u0161t\u011Bn na palub\u011B americk\u00E9ho satelitu MTI a projektu HESSI. Tato data budou porovn\u00E1v\u00E1na s na\u0161imi radiov\u00FDmi a optick\u00FDmi pozorov\u00E1n\u00EDmi. Po anal\u00FDze t\u011Bchto dat bude n\u00E1sledovat jejich modelov\u00E1n\u00ED s u\u017Eit\u00EDm ji\u017E vybudovan\u00FDch \u010Di nov\u011B vytvo\u0159en\u00FDch model\u016F. Tato data a modely umo\u017En\u00ED l\u00E9pe pochopit prim\u00E1rn\u00ED energetick\u00E9 procesy slune\u010Dn\u00EDch erupc\u00ED. Bude vybudov\u00E1n nov\u00FD hybridn\u00ED model odezvy chromosf\u00E9ry na erup\u010Dn\u00ED procesy. Bude ov\u011B\u0159ov\u00E1na na\u0161e nov\u00E1 koncepce rentgenov\u00E9ho z\u00E1\u0159en\u00ED generovan\u00E9ho neutr\u00E1ln\u00EDm svazkem i model radiov\u00E9 emise vyvr\u017Een\u00E9ho plasmoidu. Pl\u00E1nujeme prov\u00E9st modelov\u00E1n\u00ED rekonexe v pulsuj\u00EDc\u00EDm re\u017Eimu, s urychlov\u00E1n\u00EDm testuj\u00EDc\u00EDch \u010D\u00E1stic."@cs . . "4302"^^ . "solar flares; primary energy release processes; X-ray emission; radio emission; optical emission; numerical modelling"@en . "0"^^ . "Diagnostika prim\u00E1rn\u00EDch energetick\u00FDch proces\u016F ve slune\u010Dn\u00EDch erupc\u00EDch a jejich modelov\u00E1n\u00ED"@cs . .