The resolution of the pictures from the Mariner 9 mission determines the distribution of the control points, as well as the gaps in the planet-wide control net. After discussing the photogrammetric equations and the computational method used to establish the planet-wide control net and the secondary net, the camera stations and the assumed physical properties of Mars are considered. Subsequent paragraphs contain a description of the control points, their measurements, and a discussion of how distortions are removed. Finally, results of the computations are given, with tables of coordinates for the control points.


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    Titel :

    Martian surface coordinates


    Beteiligte:
    Davies, M. E. (Autor:in) / Arthur, D. W. G. (Autor:in)


    Erscheinungsdatum :

    15.07.1973


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Martian surface coordinates

    Davies, M. E. / Arthur, D. W. G. | NTRS | 1973


    Martian surface temperatures

    Morrison, D. | NTRS | 1968


    The Martian surface pressure.

    Gray, L. D. / Schorn, R. A. | NTRS | 1967


    Martian surface weathering studies

    Calvin, M. | NTRS | 1973


    The Martian Surface Boundary Layer

    Wilson, G. R. / Joshi, M. | NTRS | 2000