"Neuvedeno."@en . "\u0158e\u0161en\u00FD projekt se zab\u00FDval spektropolarimetrickou diagnostikou rychl\u00FDch proces\u016F ve slune\u010Dn\u00EDch erupc\u00EDch. \u00DAsp\u011B\u0161n\u00FD projekt zku\u0161en\u00E9ho kolektivu v\u011Bdeck\u00FDch pracovn\u00EDk\u016F ze slune\u010Dn\u00EDho odd\u011Blen\u00ED As\u00DA je dob\u0159e ilustrov\u00E1n zna\u010Dn\u00FDm po\u010Dtem kvalitn\u00EDch publikac\u00ED. Z\u00E1v\u011Bre\u010Dn\u00E1"@cs . . . "2008-05-19+02:00"^^ . "1"^^ . . "Spectropolarimetric diagnostics of fast processes in solar flares"@en . . . "Suggested project takes the advantage of high aperture, suitable spatial and extremally short temporal resolution of the Ondoejov Multichannel Flare Spectrograph for simultaneous detection of the linear polarization in the Balmer lines spectra, H-alpha filtergrams and unpolarized line profiles in solar flares using fast videocameras. The analyzed lines profiles, mainly from starting phases of solar flares, will be compared to the time records obtained by the Ondoejov Radiospectrograph and to those froman extremally hard X-ray radiation measured by the Czech-American experiment HXRS on the MTI, satellite. The results will be treated from the point of view of superthermal particles propagation in the chromosphere and also compared to the theoretically evaluated lines profiles based on NLTE models. Comparision with the results of the polarized radiation transfer in the solar flare models will be done in cooperation with colleagues from the Observatoire de Paris. We will take part in coordinated"@en . . "http://www.isvav.cz/projectDetail.do?rowId=GA205/00/1726"^^ . "26"^^ . "26"^^ . . . . . "0"^^ . . "GA205/00/1726" . . . . "Navrhovan\u00FD projekt vyu\u017E\u00EDv\u00E1 vysok\u00E9 sv\u011Btelnosti, dobr\u00E9ho \u00FAhlov\u00E9ho a extr\u00E9mn\u011B vysok\u00E9ho \u010Dasov\u00E9ho rozli\u0161en\u00ED mnohokamerov\u00E9ho spektrografu v Ond\u0159ejov\u011B k mo\u017Enosti sou\u010Dasn\u00E9 detekce line\u00E1rn\u00ED polarizace spekter Balmerovsk\u00FDch \u010Dar, H-alfa filtrogram\u016F i nepolarizovan\u00FDch profil\u016F \u010Dar ve slune\u010Dn\u00EDch erupc\u00EDch pomoc\u00ED video- kamer s kadenc\u00ED 25 sn\u00EDmk\u016F/s. Analyzovan\u00E9 profily \u010Dar, zejm\u00E9na z impulzn\u00EDch f\u00E1z\u00ED erupc\u00ED, budou porovn\u00E1ny s \u010Dasov\u00FDm z\u00E1znamem z ond\u0159ejovsk\u00E9ho radiospektrografu a s m\u011B\u0159en\u00EDm extr\u00E9mn\u011B tvrd\u00E9ho rentgenovsk\u00E9ho z\u00E1\u0159en\u00ED z \u010Desko-americk\u00E9ho dru\u017Eicov\u00E9ho experimentu HXRS. V\u00FDsledky budou interpretov\u00E1ny jak z hlediska p\u0159enosu energie nadtepeln\u00FDmi svazky elektron\u016F a proton\u016F do hust\u00FDch vrstev atmosf\u00E9ry, tak z hlediska koordinovan\u00FDch pozorovac\u00EDch kampan\u00ED sestanic\u00ED SOHO a s p\u0159ipravovanou dru\u017Eic\u00ED projektu HESSI. Navrhovan\u00FD projekt bere v \u00FAvahu aktu\u00E1ln\u00ED teoretick\u00E9 v\u00FDsledky studia energetick\u00FDch proces\u016F ve slune\u010Dn\u00EDch erupc\u00EDch s ohledem na rozli\u0161en\u00ED rol\u00ED r\u016Fzn\u00FDch mechanism\u016F p\u0159enosu energie v erupc\u00EDch. Vych\u00E1z\u00ED z" . . . "Spektropolarimetrick\u00E1 diagnostika rychl\u00FDch proces\u016F ve slune\u010Dn\u00EDch erupc\u00EDch" . . "0"^^ . .