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Laboratory measurements to interpret dust polarimetric observations and in-situ radar studies. Implications for the Rosetta mission.

Published online by Cambridge University Press:  18 July 2017

A.-Ch. Levasseur-Regourd ,
Yann Brouet  and
Edith Hadamcik
A.-Ch. Levasseur-Regourd
Affiliation:
UPMC - LATMOS - CNRS, Sorbonne Univ., BC 102, 4 place Jussieu, 75005 Paris, France email: aclr@latmos.ipsl.fr
Yann Brouet
Affiliation:
Physics Institute, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland email: yann.brouet@space.unibe.ch
Edith Hadamcik
Affiliation:
UPMC - LATMOS - CNRS, Sorbonne Univ., BC 102, 4 place Jussieu, 75005 Paris, France email: aclr@latmos.ipsl.fr
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Polarimetric astronomical observations on dust clouds and regolithic surfaces require laboratory simulations on samples to provide clues to properties of the scattering media. Similarly, in-situ radar investigations of Solar System bodies require laboratory studies to infer the physical properties of their interiors. Recent developments are illustrated by analyses of comet 67P/Churyumov-Gerasimeko (C-G) remote observations and in-situ studies from Rosetta mission.

Type
Addendum
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , E24
Copyright
Copyright © International Astronomical Union 2017 

References

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