The Space Exploration Synthetic Aperture Radar (SESAR) is a P-band (435 MHz) radar instrument for planetary applications capable of measuring the surface and subsurface of planetary bodies at full polarimetry and at meter-scale resolution. These measurements can reveal important information about the surface evolution and geologic history of the planetary bodies, and help identify buried resources for future explorers. SESAR’s architecture is based on a low power, lightweight, beamforming design, specifically developed to meet stringent requirements of planetary instruments. The SESAR developmental effort, carried out at NASA/GSFC, designed and built a prototype SAR instrument, and environmentally tested it, with the goal of maturing the SESAR technology readiness level for upcoming planetary mission opportunities.


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    Titel :

    The P-Band Space Exploration Synthetic Aperture Radar (SESAR)


    Beteiligte:
    Rafael F Rincon (Autor:in) / Lynn M Carter (Autor:in) / David Hollibaugh-Baker (Autor:in) / Cornelis F du Toit (Autor:in) / Kenneth Segal (Autor:in) / Martin Perrine (Autor:in) / Peter Steigner (Autor:in) / Iban Ibanez (Autor:in)

    Kongress:

    IEEE Radar Conference (RadarConf 2023) ; 2023 ; San Antonio, TX, US


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch




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