The evolution of the Spaceborne Imaging Radar (SIR) has lead to a multi-polarization, multifrequency synthetic aperture radar (SAR) with variable imaging geometry which will be ready for flight on the Earth Observing System (Eos) in the mid 1990's. Nominally, this SAR will be a three frequency (L-, C- and X-band) system with quadpolarization available for the L- and C-bands. It will be capable of acquiring multiincidence angle data using electronic beam steering and other imaging geometries by mechanically pitching, yawing and rolling the antenna. The Eos SAR will provide a unique new data set and will play a key role along with the other Eos instruments in understanding the Earth as a global system.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    The spaceborne imaging radar experiments


    Weitere Titelangaben:

    Untersuchungen am Abbildungsradar fuer den Weltraum (SIR)


    Beteiligte:
    Cimino, J.B. (Autor:in)


    Erscheinungsdatum :

    1987


    Format / Umfang :

    7 Seiten, 2 Bilder, 10 Quellen


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Print


    Sprache :

    Englisch





    Spaceborne Imaging Radar Project

    Herman, Neil | NTRS | 1986


    Spaceborne Imaging Radar Project

    N. Herman | NTIS | 1986


    Spaceborne Imaging Radar Symposium

    C. Elachi | NTIS | 1983


    Spaceborne Imaging Radar Symposium

    Elachi, C. | NTRS | 1983