Planck polarimetry: modeling the galactic magnetic field.

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Planck polarimetry: modeling the galactic magnetic field.

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2010-06

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I created a model of polarized emission from dust grains aligned with the galactic magnetic field for comparison with Planck observations. I modeled the magnetic field in the galactic disk as a field with a cylindrical constant component and an equal strength random component. I investigated how the fractional polarization down a line of sight varies with different models of a random field. I determine that different models of random fields yield different amounts of fractional polarization, especially over sightlines longer than a decorrelation length.

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University of Minnesota M.S. thesis. June 2010. Major: Astrophysics. Advisor: Terry J. Jones. 1 computer file (PDF); vii, 30 pages. Ill. (some col.)

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Wahl, Theodore Park. (2010). Planck polarimetry: modeling the galactic magnetic field.. Retrieved from the University Digital Conservancy, https://hdl.handle.net/11299/93535.

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