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<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/"><rdf:Description rdf:about="https://repozitorij.uni-lj.si/IzpisGradiva.php?id=117346"><dc:title>Analysis of solar flare timing in radio and X-ray bands</dc:title><dc:creator>Brešan,	Andrej	(Avtor)
	</dc:creator><dc:creator>Zwitter,	Tomaž	(Mentor)
	</dc:creator><dc:creator>Messerotti,	Mauro	(Komentor)
	</dc:creator><dc:subject>solar flares</dc:subject><dc:subject>magnetic reconnection</dc:subject><dc:subject>radio astronomy</dc:subject><dc:subject>standard model of solar flares</dc:subject><dc:subject>X-rays</dc:subject><dc:subject>trieste solar radio system</dc:subject><dc:subject>GOES satellites</dc:subject><dc:subject>solar energetic particles</dc:subject><dc:subject>solar flare statistics</dc:subject><dc:subject>solar flare radio precursors</dc:subject><dc:subject>experimental radio telescope</dc:subject><dc:description>This thesis presents the standard solar flare model and one of the possible verifications of its validity by analyzing radio-solar data taken with the Trieste Solar Radio System (TSRS), located near the city of Trieste in Italy. A review of measured data was made based on a list of solar energetic particle (SEP) events, produced by solar flares in the years between 1996 and 2016. Features expected for bursts produced by a flare following the standard model --- namely peaking times in six radio frequencies and two X-ray bands --- were observed. The majority of observed events showed a fair congruence with the expected time sequence of peaks in the standard flare model. However, many exceptions to the standard model rules and complex events were also identified, necessitating further investigation. The events were subsequently gathered in order to obtain a statistical overview of radio and X-ray peaks time delays that was compared to previous works performed by other research groups. We found our findings to correspond broadly to theirs. Next, we verified how many SEP events were preceded by a solar radio burst observed in Trieste. We sought to confirm the reliability of our instrument for identifying potentially hazardous solar events, finding four such events. In the end, we described a feature observed in the TSRS data which could represent a precursor event for large solar flares. The theory would require confirmation or rejection in future analyses. As part of work on this thesis, an experimental radio telescope project was started by the author and his colleagues. This project is outlined in brief in the conclusion as a supplement to the thesis.</dc:description><dc:date>2020</dc:date><dc:date>2020-07-08 08:15:02</dc:date><dc:type>Magistrsko delo/naloga</dc:type><dc:identifier>117346</dc:identifier><dc:language>sl</dc:language></rdf:Description></rdf:RDF>
