Electron acceleration at localized wave structures in the solar corona [Elektronische Ressource] / von Rositsa Stoycheva Miteva

Astrophysikalisches Institut PotsdamArbeitsgruppe Solare Radiophysik———————————————————————————————————Electron acceleration at localized wave structuresin the solar coronaDissertationzur Erlangung des akademischen Grades‘doctor rerum naturalium’(Dr. rer. nat.)in der Wissenschaftsdisziplin ‘Astrophysik’eingereicht an derMathematisch–Naturwissenschaftlischen Fakult¨atder Universit¨at PotsdamvonRositsa Stoycheva MitevaPotsdam, im M¨arz 2007This work is licensed under the Creative Commons Attribution-Noncommercial-No Derivative Works 3.0 License. To view a copy of this license, visit http://creativecommons.org/licenses/by-nc-nd/3.0/ or send a letter to Creative Commons, 171 Second Street, Suite 300, San Francisco, California, 94105, USA. Elektronisch veröffentlicht auf dem Publikationsserver der Universität Potsdam: http://opus.kobv.de/ubp/volltexte/2007/1477/ urn:nbn:de:kobv:517-opus-14775 [http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-14775] Thesis advisor AuthorProf. Dr. Gottfried Mann Rositsa Stoycheva MitevaElectron acceleration at localized wave structures in the solar coronaAbstractThe Sun is an active star that manifests its activity not only in the appearance of the well-known sunspots but also in flares. During a flare, a huge amount of the stored magneticenergy is suddenly released and transfered into: a local heating of the corona, mass motions(e.g.