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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
Extract
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