Production mechanism of cocmic rays by supernova remnants

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dc.contributor.advisorHektor, Andi, juhendaja
dc.contributor.advisorRaidal, Martti, juhendaja
dc.contributor.advisorStrumia, Alessandro, juhendaja
dc.contributor.authorTuvi, Taavi
dc.contributor.otherTartu Ülikool. Loodus- ja tehnoloogiateaduskondet
dc.contributor.otherTartu Ülikool. Füüsika instituutet
dc.date.accessioned2014-06-11T12:32:28Z
dc.date.available2014-06-11T12:32:28Z
dc.date.issued2014
dc.description.urihttps://www.ester.ee/record=b4095440*estet
dc.identifier.urihttp://hdl.handle.net/10062/41723
dc.language.isoenen
dc.publisherTartu Ülikoolet
dc.subject.othermagistritöödet
dc.subject.otherkosmiline kiirguset
dc.subject.othersupernoovadet
dc.subject.othermodelleerimine (teadus)et
dc.titleProduction mechanism of cocmic rays by supernova remnantset
dc.typeThesisen

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Füüsika õppekava magistritööd – Master's theses