SAEMPL

Scattering and absorption of electromagnetic waves in particulate media

Coordinatore	HELSINGIN YLIOPISTO    more Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie.
Nazionalità Coordinatore	Finland [FI]
Totale costo	2˙749˙532 €
EC contributo	2˙749˙532 €
Programma	FP7-IDEAS-ERC Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	ERC-2012-ADG_20120216
Funding Scheme	ERC-AG
Anno di inizio	2013
Periodo (anno-mese-giorno)	2013-04-01   -   2018-03-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	HELSINGIN YLIOPISTO  Organization address address: YLIOPISTONKATU 4 city: HELSINGIN YLIOPISTO postcode: 14 contact info Titolo: Ms. Nome: Satu Cognome: Väisänen Email: send email Telefono: +358 9 191 50613 Fax: +358 9 191 51080	FI (HELSINGIN YLIOPISTO)	hostInstitution	2˙749˙532.00
2	HELSINGIN YLIOPISTO  Organization address address: YLIOPISTONKATU 4 city: HELSINGIN YLIOPISTO postcode: 14 contact info Titolo: Prof. Nome: Karri Olavi Cognome: Muinonen Email: send email Telefono: +358 9 19122941 Fax: +358 9 19150610	FI (HELSINGIN YLIOPISTO)	hostInstitution	2˙749˙532.00

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 Obiettivo del progetto (Objective)

'The canonical problem of electromagnetic scattering in complex particulate media is solved numerically using multiple-scattering theory based on the Maxwell equations, with an exact treatment of the leading ladder and cyclical interaction diagrams. The numerical methods are validated using a nanotechnology-based scattering experiment that, simultaneously with the measurement of the full scattering matrix at arbitrary illumination and observation geometries, allows for a detailed physical characterization of the scattering object using Atomic Force Microscopy. The numerical and experimental methods will have a major impact on how knowledge is accrued on objects in our Solar System based on their scattering characteristics, with wavelengths spanning from the ultraviolet to radio, using both space-based and ground-based observing programs. The methods will have immediate applications in Earth observation, including remote sensing of the atmosphere, land, and sea.'