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Challenges for Hapke modeling of asteroid reflectance spectra in the mid-infrared range

Silva, C M and Seixas, T.A. and Sazonov, Pavlo and Maturilli, Alessandro and Helbert, Jörn (2018) Challenges for Hapke modeling of asteroid reflectance spectra in the mid-infrared range. EGU 2018, 8. - 13. Apr. 2018, Wien, Austria.

Full text not available from this repository.

Official URL: https://meetingorganizer.copernicus.org/EGU2018/EGU2018-19738.pdf

Abstract

Hapke’s radiative transfer theory provides a complete framework for modeling bi-directional reflectance (BDR) spectra of minerals and intimate mixtures of minerals, as those forming asteroidal regoliths. There are, however, some factors that may render questionable the use of Hapke’s model to retrieve grain size and abundance of each component mineral from BDR spectra. In particular, the assumption of a wavelength-independent phase function, which has been routinely used for BDR spectra in the UV-VIS-NIR range, is still to be tested in a wider wavelength range. This is an absolute requirement because dramatic changes in light absorption and scattering are likely to occur near anomalies in the refraction index in the mid-infrared (MIR) range. We performed BDR spectroscopy measurements on single mineral assemblages of olivine (OL) and augite (AUG) minerals in the wavelength range 0.3-18 mm and for several phase angles. The measured spectra, which show evidence for a wavelength-dependent phase function, were fitted using Happke’s model with phase functions of Legendre and Henyey-Greenstein types with variable coefficients. It is found that fitting the quasi-isotropic scattering features and the inversion of radiance vs phase angle monotonicity, which are observed both OL and AUG assemblages, requires modeling the phase function with Legendre polynomials of order 5, at least; moreover, the coefficients of these polynomials depend linearly on wavelength. We present the results of this analysis and its consequences for Hapke’s modeling of asteroid reflectance spectra in the MIR range.

Item URL in elib:https://elib.dlr.de/124762/
Document Type:Conference or Workshop Item (Speech)
Title:Challenges for Hapke modeling of asteroid reflectance spectra in the mid-infrared range
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Silva, C MFaculdade de Ciências, Universidade de Lisboa, 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
Sazonov, PavloCenter for Earth and Space Research of University of Coimbra (CITEUC), PortugalUNSPECIFIED
Maturilli, AlessandroAlessandro.Maturilli (at) dlr.deUNSPECIFIED
Helbert, JörnJoern.Helbert (at) dlr.dehttps://orcid.org/0000-0001-5346-9505
Date:April 2018
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:Hapke, PSL, reflectance
Event Title:EGU 2018
Event Location:Wien, Austria
Event Type:international Conference
Event Dates:8. - 13. Apr. 2018
Organizer:EGU
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: Maturilli, Alessandro
Deposited On:11 Dec 2018 09:17
Last Modified:11 Dec 2018 09:17

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