The objectives of the Apollo 17 Lunar Sounder Experiment (ALSE) were to detect subsurface geologic structures, to generate a continuous lunar profile, and to image the moon at radar wavelengths. A three-wavelength synthetic-aperture radar (SAR) operating at 60, 20, and 2 m wavelengths was designed to attain these objectives. The design choices reflected a balance of scientific requirements versus Apollo mission and hardware constraints. The radar data from the lunar mission were recorded on photographic film in a conventional SAR format, and were returned to earth for processing. A combination of optical and digital processing and exploitation techniques was applied to the scientific interpretation of the data. Some preliminary results from the lunar mission have been obtained.


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    Titel :

    The Apollo Lunar Sounder radar system


    Beteiligte:
    Porcello, L. J. (Autor:in) / Zelenka, J. S. (Autor:in) / Adams, G. F. (Autor:in) / Jackson, P. L. (Autor:in) / Jordan, R. L. (Autor:in) / Phillips, R. J. (Autor:in) / Brown, W. E., Jr. (Autor:in) / Ward, S. H. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.06.1974


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Apollo lunar sounder experiment

    Phillips, R. J. / Adams, G. F. / Brown, W. E., Jr. et al. | NTRS | 1973


    The Apollo 17 Lunar Sounder

    Phillips, R. J. / Brown, W. E., Jr. / Jordan, R. et al. | NTRS | 1973


    The Apollo 17 Lunar Sounder.

    Phillips, R. J. / Brown, W. E., Jr. / Ward, S. H. | NTRS | 1973