Copyright © Björn J. R. Davidsson 2008. Duplication of the contents of this page, in whole or
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DIPLOMA THESIS PROJECTS
If you are a student at Uppsala University who wish to write a Master of Science diploma
thesis you may consider the following project, having me as your supervisor. Contact
information can be found on the main page.
Thermal Emission of Cometary Dust Grains
The mineralogical composition of cometary dust particles is often determined
by analyzing thermal emission spectra of cometary comae obtained by spaceborne observatories.
Classically, synthetic spectra of spherical single-component grains are calculated for different
minerals and grain sizes. By combining such synthetic spectra and requiring that the observed
spectra thereby are reproduced, one can determine the composition of cometary dust grains
and the relative abundances of different species. In reality, however, comet dust grains are
non-spherical and consist of intimately mixed minerals, which means that the classical procedure
is inaccurate. The project consist of investigating the severity of such inaccuracies by performing
light scattering and thermal emission calculations for non-spherical multi-component dust
grains, using state-of-the-art software.
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