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Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog

Published online by Cambridge University Press:  05 March 2015

Frédérick Poidevin
Affiliation:
University College London, Kathleen Lonsdale Building, Department of Physics & Astronomy, Gower Place, London WC1E 6BT, United Kingdom email: Poidevin@star.ucl.ac.uk
Diego Falceta-Gonçalves
Affiliation:
University College London, Kathleen Lonsdale Building, Department of Physics & Astronomy, Gower Place, London WC1E 6BT, United Kingdom email: Poidevin@star.ucl.ac.uk
Grzegorz Kowal
Affiliation:
University College London, Kathleen Lonsdale Building, Department of Physics & Astronomy, Gower Place, London WC1E 6BT, United Kingdom email: Poidevin@star.ucl.ac.uk
Elisabete De Gouveia Dal Pino
Affiliation:
University College London, Kathleen Lonsdale Building, Department of Physics & Astronomy, Gower Place, London WC1E 6BT, United Kingdom email: Poidevin@star.ucl.ac.uk
Antonio-Mário Magalhães
Affiliation:
University College London, Kathleen Lonsdale Building, Department of Physics & Astronomy, Gower Place, London WC1E 6BT, United Kingdom email: Poidevin@star.ucl.ac.uk
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Abstract

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The SCUPOL catalog is a compilation of 83 regions that were observed at the JCMT between 1997 and 2005. For sufficiently sampled maps, we conduct an analysis for characterizing the polarization and magneto-turbulent properties of the observed regions. The same analysis is done on 2D polarization maps produced by 3D MHD 1024 pixel grid simulations that have been scaled on a sample of observed maps. Each scaled MHD cube of simulated data is used to calculate the mean turbulent regime of each observed regions.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

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