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Coronal Holes and Solar f-Mode Wave Scattering Off Linear Boundaries

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dc.contributor.advisor Weigel, RobertPesnell, William D
dc.contributor.author Hess Webber, Shea A.
dc.creator Hess Webber, Shea A.
dc.date.accessioned 2017-01-29T01:16:38Z
dc.date.available 2017-01-29T01:16:38Z
dc.date.issued 2016
dc.identifier.uri http://hdl.handle.net/1920/10603
dc.description.abstract Coronal holes (CHs) are solar atmospheric features that have reduced emission in the extreme ultraviolet (EUV) spectrum due to decreased plasma density along open magnetic field lines. CHs are the source of the fast solar wind, can influence other solar activity, and track the solar cycle. Our interest in them deals with boundary detection near the solar surface. Detecting CH boundaries is important for estimating their size and tracking their evolution through time, as well as for comparing the physical properties within and outside of the feature.
dc.format.extent 234 pages
dc.language.iso en
dc.rights Copyright 2016 Shea A. Hess Webber
dc.subject Astrophysics
dc.subject Physics
dc.subject Coronal Holes
dc.subject Solar Physics
dc.subject Space Weather
dc.subject Time-Distance Helioseismology
dc.title Coronal Holes and Solar f-Mode Wave Scattering Off Linear Boundaries
dc.type Dissertation
thesis.degree.level Ph.D.
thesis.degree.discipline Computational Sciences and Informatics
thesis.degree.grantor George Mason University


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