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Solar proton radiation during an interplanetary space mission

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dc.contributor Aran i Sensat, Maria dels Àngels
dc.creator Florido Llinàs, Robert
dc.date 2018-09-13T15:28:15Z
dc.date 2018-09-13T15:28:15Z
dc.date 2018-01
dc.date.accessioned 2024-12-16T10:26:39Z
dc.date.available 2024-12-16T10:26:39Z
dc.identifier http://hdl.handle.net/2445/124534
dc.identifier.uri http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/21401
dc.description Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutora: Àngels Aran Sensat
dc.description SEPs events are a serious hazard for both spacecraft and humans during interplanetary space missions. In this work, we use the ESA's SEPEM tool for statistical modelling the cumulative and the worst case proton fluences over the missions Helios 1 and Helios 2. We compute their energy spectra for periods of the solar cycle over the mission duration and fit them to most common distributions. We analyse the best fitting function for each case. Finally, we compare the cumulative fluence energy spectra of the model results at a 90% confidence level with data measured by the Helios 1 and 2 spacecraft.
dc.format 5 p.
dc.format application/pdf
dc.language eng
dc.rights cc-by-nc-nd (c) Florido, 2018
dc.rights http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights info:eu-repo/semantics/openAccess
dc.source Treballs Finals de Grau (TFG) - Física
dc.subject Radiació solar
dc.subject Protons
dc.subject Treballs de fi de grau
dc.subject Solar radiation
dc.subject Protons
dc.subject Bachelor's theses
dc.title Solar proton radiation during an interplanetary space mission
dc.type info:eu-repo/semantics/bachelorThesis


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