The diversity of landforms visible in the Viking images of Mars have led to a proliforation of geomorphic agents proposed to be active in shaping the Martian surface. While it is likely that numerous different processes have contributed to the geomorphology of Mars throughout Martian history, it is important that proposed Martian geomorphic agents be subjected to critical scrutiny by the scientific community. High resolution Viking Orbiter images represent a data set for investigating geomorphic processes on Mars. Geologic mapping of Mars can take place at a variety of scales, utilizing a variety of image resolutions, but an interpretation of the history of individual landforms is dependent upon the best available spatial resolution. These high resolution images provide the opportunity to examine proposed Martian geomorphic processes. It is clear that researchers may not interpret features in the same way but it is important that high resolution images of candidate features be made available to the scientific community so that a consensus can be reached. This procedure can provide a way to refine the understanding of geomorphic processes on Mars.


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    Titel :

    High resolution Viking Orbiter images: A useful data source for testing the viability of geomorphic processes attributed to Martian landforms


    Beteiligte:


    Erscheinungsdatum :

    1987-01-01


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch





    A Catalog of Selected Viking Orbiter Images

    Turner, R. L. / Carroll, R. D. | NTRS | 1983


    Viking Orbiter Stereo Imaging Catalog

    K. R. Blasius / A. V. Vertrone / B. H. Lewis et al. | NTIS | 1982


    Viking Orbiter Stereo Imaging Catalog

    K. R. Blasius / A. V. Vetrone / M. D. Martin | NTIS | 1980


    IPL Processing of the Viking Orbiter Images of Mars

    Ruiz, R. M. / Elliott, D. A. / Yagi, G. M. et al. | NTRS | 1977