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Properties of the Orionid meteors observed in 2006
dc.contributor.advisorKoten, Pavel
dc.creatorVojáček, Vlastimil
dc.date.accessioned2017-04-20T15:40:08Z
dc.date.available2017-04-20T15:40:08Z
dc.date.issued2009
dc.identifier.urihttp://hdl.handle.net/20.500.11956/27360
dc.description.abstractIn the present work we study the Orionid 2006 meteor shower. All results in this work come from double station video observations. We study exceptional activity, caused most probably by particles trapped in resonance motion with Jupiter. We focused on light curves, atmospheric trajectories and orbital elements of meteoroids. We can find here comparison with other years of activity of the Orionid meteor shower and comparison with other annual meteor showers.en_US
dc.languageČeštinacs_CZ
dc.language.isocs_CZ
dc.publisherUniverzita Karlova, Matematicko-fyzikální fakultacs_CZ
dc.titleVlastnosti Orionid pozorovaných v roce 2006cs_CZ
dc.typediplomová prácecs_CZ
dcterms.created2009
dcterms.dateAccepted2009-09-15
dc.description.departmentAstronomical Institute of Charles Universityen_US
dc.description.departmentAstronomický ústav UKcs_CZ
dc.description.facultyFaculty of Mathematics and Physicsen_US
dc.description.facultyMatematicko-fyzikální fakultacs_CZ
dc.identifier.repId61675
dc.title.translatedProperties of the Orionid meteors observed in 2006en_US
dc.contributor.refereeŠolc, Martin
dc.identifier.aleph001139375
thesis.degree.nameMgr.
thesis.degree.levelnavazující magisterskécs_CZ
thesis.degree.disciplineAstronomie a astrofyzikacs_CZ
thesis.degree.disciplineAstronomy and Astrophysicsen_US
thesis.degree.programFyzikacs_CZ
thesis.degree.programPhysicsen_US
uk.thesis.typediplomová prácecs_CZ
uk.taxonomy.organization-csMatematicko-fyzikální fakulta::Astronomický ústav UKcs_CZ
uk.taxonomy.organization-enFaculty of Mathematics and Physics::Astronomical Institute of Charles Universityen_US
uk.faculty-name.csMatematicko-fyzikální fakultacs_CZ
uk.faculty-name.enFaculty of Mathematics and Physicsen_US
uk.faculty-abbr.csMFFcs_CZ
uk.degree-discipline.csAstronomie a astrofyzikacs_CZ
uk.degree-discipline.enAstronomy and Astrophysicsen_US
uk.degree-program.csFyzikacs_CZ
uk.degree-program.enPhysicsen_US
thesis.grade.csVýborněcs_CZ
thesis.grade.enExcellenten_US
uk.abstract.enIn the present work we study the Orionid 2006 meteor shower. All results in this work come from double station video observations. We study exceptional activity, caused most probably by particles trapped in resonance motion with Jupiter. We focused on light curves, atmospheric trajectories and orbital elements of meteoroids. We can find here comparison with other years of activity of the Orionid meteor shower and comparison with other annual meteor showers.en_US
uk.publication.placePrahacs_CZ
uk.grantorUniverzita Karlova, Matematicko-fyzikální fakulta, Astronomický ústav UKcs_CZ
dc.identifier.lisID990011393750106986


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