SAEMPL

Scattering and absorption of electromagnetic waves in particulate media

 Coordinatore HELSINGIN YLIOPISTO 

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

Mappa


 Word cloud

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observation    scattering    numerical   

 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.'

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