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VIRTIS emissivity of Alpha Regio, Venus, with implications for tessera composition

Gilmore, M. and Müller, Nils and Helbert, Jörn (2015) VIRTIS emissivity of Alpha Regio, Venus, with implications for tessera composition. Icarus: International Journal of Solar System Studies (254), pp. 350-361. Elsevier. DOI: 10.1016/j.icarus.2015.04.008 ISSN 0019-1035

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Official URL: http://www.sciencedirect.com/science/article/pii/S0019103515001438

Abstract

The 1 μm emissivity of Alpha Regio tessera is lower than adjacent plains. The emissivity is due to material properties such as composition or grain size. The emissivity data are consistent with felsic compositions or basaltic weathering. Such mineralogy may record an extinct era of Venus history

Item URL in elib:https://elib.dlr.de/101759/
Document Type:Article
Title:VIRTIS emissivity of Alpha Regio, Venus, with implications for tessera composition
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Gilmore, M.Wesleyan Univ., USAUNSPECIFIED
Müller, NilsNils.Mueller (at) dlr.deUNSPECIFIED
Helbert, JörnJoern.Helbert (at) dlr.dehttps://orcid.org/0000-0001-5346-9505
Date:July 2015
Journal or Publication Title:Icarus: International Journal of Solar System Studies
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:Yes
In ISI Web of Science:Yes
DOI :10.1016/j.icarus.2015.04.008
Page Range:pp. 350-361
Publisher:Elsevier
ISSN:0019-1035
Status:Published
Keywords:Venus, surface; Spectroscopy; Mineralogy
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 Venus Express Kamera (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Leitungsbereich PF
Deposited By: Maturilli, Alessandro
Deposited On:07 Jan 2016 09:50
Last Modified:01 Dec 2018 19:51

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