Computational Intelligence Techniques for Submillimetre Polarization Modeling

Details Computational Intelligence Techniques for Submillimetre Polarization Modeling Computational Intelligence Techniques for Submillimetre Polarization Modeling

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..343..171f&link_type=abstract

Astronomical Polarimetry: Current Status and Future Directions ASP Conference Series, Vol. 343, Proceedings of the Conference he

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Detailed modeling of submillimetre continuum and polarization data in the submillimetre involves a massive-scale parameter search to optimize fits to continuum and polarization data simultaneously. We introduce a new modeling technique based on an advanced multi-objective genetic algorithm that solves these problems very efficiently. We model the 850 micron continuum emission of the G11.11-0.12 filamentary infrared dark cloud, and predict the corresponding polarization patterns. We also show preliminary fits to the continuum and polarized emission of a clump within the OMC-3 region of the Orion filament. Finally, we discuss how this technique might be used to model the large polarization data sets that future SCUBA-2 molecular cloud surveys would produce.

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