Spectro-polarimetry as a tool for characterizing small cosmic dust grains

DOI: 
Publication date: 
01/09/2017
Main author: 
Muñoz, O.
IAA authors: 
Muñoz, O.;Moreno, F.;Escobar-Cerezo, J.;Guirado, D.
Authors: 
Muñoz, O.;Moreno, F.;Escobar-Cerezo, J.;Guirado, D.
Journal: 
European Planetary Science Congress
Refereed: 
No
Publication type: 
Article
Volume: 
11
Pages: 
EPSC2017
Abstract: 

In this work we show how experimental data of intensity and polarization of the scattered light of different cosmic dust analogues can be used to shed some light on the nature of dust particles. The experimental data are performed at various wavelengths (447, 520 and 647 nm) covering the scattering angle range from 3 to 177 degrees.

Database: 
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2017EPSC...11..325M/abstract
ADS Bibcode: 
2017EPSC...11..325M