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application to Martian dust tori and Enceladus dust plumes

dc.contributor.authorMakuch, Martin
dc.date.accessioned2010-10-12T18:23:18Z
dc.date.available2010-10-12T18:23:18Z
dc.date.issued2007
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0001-30DD-5
dc.description.abstractOur Solar system contains a large amount of dust, containing valuable information about our close cosmic environment. If created in a planet's system, the particles stay predominantly in its vicinity and can form extended dust envelopes, tori or rings around them. A fascinating example of these complexes are Saturnian rings containing a wide range of particles sizes from house-size objects in the main rings up to micron-sized grains constituting the E ring. Other example are ring systems in general, containing a large fraction of dust or also the putative dust-tori surrounding the planet Mars. The dynamical life'' of such circumplanetary dust populations is the main subject of our study...
dc.format.extent115, 10 Bl.
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherUniv. Potsdam
dc.rights.urihttp://e-docs.geo-leo.de/rights
dc.subject.ddc523
dc.subject.gokTGL 800
dc.titleCircumplanetary dust dynamics
dc.title.alternativeapplication to Martian dust tori and Enceladus dust plumes
dc.typemonograph
dc.subject.gokverbalInterplanetarer Staub {Astronomie}
dc.identifier.doi10.23689/fidgeo-87
dc.identifier.ppn53871493X
dc.type.versionpublishedVersion
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


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