The Pointed Telescope Subassembly (PTS) consists of a telescope, its Coude relay optics, a two axis gimbal mechanism, and a cover/caging device. These components, their mechanisms, the requirements, and some of the trade-offs leading to the final design are described. The PTS supplies light to the interferometer of the High Resolution Doppler Imager to be used to study upper atmospheric wind velocity.


    Access

    Access via TIB

    Check availability in my library


    Export, share and cite



    Title :

    Pointed telescope subassembly for the UARS High Resolution Doppler Imager


    Contributors:


    Publication date :

    1987-05-01


    Type of media :

    Conference paper


    Type of material :

    No indication


    Language :

    English




    Stellar Alignment of the High Resolution Doppler Imager

    Marshall, A.R. | Online Contents | 1995


    Stellar alignment of the High Resolution Doppler Imager

    Marshall, Alan R. / Gell, David A. / Yee, Jeng-Hwa et al. | AIAA | 1995


    Atmospheric wind measurements with the high-resolution Doppler imager

    Grassl, Heinz J. / Skinner, Wilbert R. / Hays, Paul B. et al. | AIAA | 1995