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Emissivity and Reflectance Spectra of Asteroid analogs: their dependence on emerging angle.

Maturilli, Alessandro and Helbert, Jörn and D'Amore, Mario and Ferrari, Sabrina (2014) Emissivity and Reflectance Spectra of Asteroid analogs: their dependence on emerging angle. AGU 2014, 15.-19. Dez. 2014, San Francisco, Kalifornien.

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Abstract

At the Planetary Emissivity Laboratory (PEL) of DLR in Berlin we set-up an experiment to measure the emissivity of two asteroid analogs, fine powdered (<25 µm) meteorite Millbillillie and a synthetic enstatite at surface temperature of 373K, with emerging angle (e) from 0° to 60°, with 10° step intervals.

Item URL in elib:https://elib.dlr.de/93520/
Document Type:Conference or Workshop Item (Poster)
Title:Emissivity and Reflectance Spectra of Asteroid analogs: their dependence on emerging angle.
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Maturilli, AlessandroAlessandro.Maturilli (at) dlr.deUNSPECIFIED
Helbert, JörnJoern.Helbert (at) dlr.dehttps://orcid.org/0000-0001-5346-9505
D'Amore, MarioMario.DAmore (at) dlr.dehttps://orcid.org/0000-0001-9325-6889
Ferrari, Sabrinasabrina.ferrari (at) dlr.deUNSPECIFIED
Date:December 2014
Refereed publication:No
Open Access:Yes
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:emissivity emergence angle asteroids
Event Title:AGU 2014
Event Location:San Francisco, Kalifornien
Event Type:international Conference
Event Dates:15.-19. Dez. 2014
Organizer:AGU
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):R - Vorhaben Exploration des Sonnensystems
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Experimentelle Planetenphysik
Deposited By: Maturilli, Alessandro
Deposited On:18 Dec 2014 09:30
Last Modified:31 Jul 2019 19:50

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