Accurate photometric reconstruction of the Lunar surface is important in the context of upcoming NASA robotic missions to the Moon and in giving a more accurate understanding of the Lunar soil composition. This paper describes a novel approach for joint estimation of Lunar albedo, camera exposure time, and photometric parameters that utilizes an accurate Lunar-Lambertian reflectance model and previously derived Lunar topography of the area visualized during the Apollo missions. The method introduced here is used in creating the largest Lunar albedo map (16% of the Lunar surface) at the resolution of 10 meters/pixel.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    Photometric Lunar Surface Reconstruction


    Beteiligte:
    Nefian, Ara V. (Autor:in) / Alexandrov, Oleg (Autor:in) / Morattlo, Zachary (Autor:in) / Kim, Taemin (Autor:in) / Beyer, Ross A. (Autor:in)

    Kongress:

    International Conference on Image Processing (ICIP) ; 2013 ; Melbourne, Australia, Australia


    Erscheinungsdatum :

    2013-09-15


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch




    Photometric Lunar Surface Reconstruction

    A. V. Nefian / O. Alexandrov / Z. Morattlo et al. | NTIS | 2013


    The lunar photometric function

    BURKHARD, D. / SEXL, R. | AIAA | 1969