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Behaviour of phase functions of Olivine and Augite assemblages in the wavelength range 0.3-18 μm

Salgueiro da Silva, M.A. and Seixas, T.A. and Maturilli, Alessandro and Helbert, Jörn (2017) Behaviour of phase functions of Olivine and Augite assemblages in the wavelength range 0.3-18 μm. European Planetary Science Congress 2017, 17.-22. Sept. 2017, Riga, Lettland.

Full text not available from this repository.


Item URL in elib:https://elib.dlr.de/116300/
Document Type:Conference or Workshop Item (Speech)
Title:Behaviour of phase functions of Olivine and Augite assemblages in the wavelength range 0.3-18 μm
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Salgueiro da Silva, M.A.Department of Physics and Astronomy, Faculty of Science, University of Porto, Porto, Portugal ; Center for Earth and Space Research of University of Coimbra (CITEUC), Coimbra, PortugalUNSPECIFIED
Seixas, T.A.Department of Physics and Astronomy, Faculty of Science, University of Porto, Porto, Portugal ; Center for Earth and Space Research of University of Coimbra (CITEUC), Coimbra, PortugalUNSPECIFIED
Maturilli, AlessandroAlessandro.Maturilli (at) dlr.deUNSPECIFIED
Helbert, JörnJoern.Helbert (at) dlr.dehttps://orcid.org/0000-0001-5346-9505
Date:September 2017
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:phase function remote sensing hapke model
Event Title:European Planetary Science Congress 2017
Event Location:Riga, Lettland
Event Type:international Conference
Event Dates:17.-22. Sept. 2017
Organizer:EPSC
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Science and Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Erforschung des Weltraums
DLR - Research theme (Project):Projekt BepiColombo MERTIS und BELA
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Leitungsbereich PF
Deposited By: Helbert, Dr.rer.nat. Jörn
Deposited On:30 Nov 2017 11:13
Last Modified:30 Nov 2017 11:13

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