Synthetic spectrum methods for three dimensional supernova models.

dc.contributor.advisorBranch, David,en_US
dc.contributor.authorThomas, Rollin Corwin.en_US
dc.date.accessioned2013-08-16T12:19:00Z
dc.date.available2013-08-16T12:19:00Z
dc.date.issued2003en_US
dc.description.abstractThis dissertation describes some problems associated with synthesizing emergent spectra from three-dimensional supernova envelope models. We confront these problems by developing a three-dimensional implementation of a hybrid Sobolev/Monte Carlo technique. A collection of experiments (extending from the illustrative to the more detailed) are included.en_US
dc.format.extentxiii, 153 leaves :en_US
dc.identifier.urihttp://hdl.handle.net/11244/615
dc.noteAdviser: David Branch.en_US
dc.noteSource: Dissertation Abstracts International, Volume: 64-06, Section: B, page: 2716.en_US
dc.subjectStars Spectra.en_US
dc.subjectPhysics, Astronomy and Astrophysics.en_US
dc.subjectStars Atmospheres.en_US
dc.subjectSupernovae Models.en_US
dc.thesis.degreePh.D.en_US
dc.thesis.degreeDisciplineHomer L. Dodge Department of Physics and Astronomyen_US
dc.titleSynthetic spectrum methods for three dimensional supernova models.en_US
dc.typeThesisen_US
ou.groupCollege of Arts and Sciences::Homer L. Dodge Department of Physics and Astronomy
ou.identifier(UMI)AAI3093583en_US

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