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Modelling reflected polarized light from exoplanetary atmospheres
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy. (Astronomi och rymdfysik)
2011 (English)Independent thesis Advanced level (degree of Master (Two Years)), 20 credits / 30 HE creditsStudent thesis
Abstract [en]

I present numerical simulations of intensity and degree of polarization of light reflected by Earth-like exoplanets. The results are presented as a function of wavelength, and for a few different phase angles and a few different points on the planet. At this stage the aim is to show the working code and test a few different set ups of the star-planet system in order to find preferable configurations for observations. Not surprisingly, phase angle 90◦ shows the largest degree of polarization. For beneficial wavelength regions, visual light shows a larger overall degree of polarization, while NIR shows very clear absorption patterns in the degree of polarization, making detection of the atmospheric composition possible.

Place, publisher, year, edition, pages
2011. , 35 p.
Series
FYSAST
Keyword [en]
polarized light, polarization, atmosphere, spectrum, EXO planet, extra solar planet, planet, star, atmospheric features
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:uu:diva-173451OAI: oai:DiVA.org:uu-173451DiVA: diva2:523808
Educational program
Master Programme in Physics
Uppsok
Physics, Chemistry, Mathematics
Supervisors
Examiners
Available from: 2012-05-07 Created: 2012-04-24 Last updated: 2012-05-07Bibliographically approved

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fulltext(550 kB)334 downloads
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CiteExportLink to record
Permanent link

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Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf