SuperHERO is a hard x-ray (20-75 keV) balloon-borne telescope, currently in its proposal phase, that will utilize high angular-resolution grazing-incidence optics, coupled to novel CdTe multi-pixel, fine-pitch (250 micrometers) detectors. The high-resolution electroformed-nickel, grazing-incidence optics were developed at MSFC, and the detectors were developed at the Rutherford Appleton Laboratory in the UK, and are being readied for flight at GSFC. SuperHERO will use two active pointing systems; one for carrying out astronomical observations and another for solar observations during the same flight. The telescope will reside on a light-weight, carbon-composite structure that will integrate the Wallops Arc Second Pointer into its frame, for arcsecond or better pointing. This configuration will allow for Long Duration Balloon flights that can last up to 4 weeks. This next generation design, which is based on the High Energy Replicated Optics (HERO) and HERO to Explore the Sun (HEROES) payloads, will be discussed, with emphasis on the core telescope components.


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    Titel :

    SuperHERO: Design of a New Hard X-Ray Focusing Telescope


    Beteiligte:
    Gaskin, Jessica (Autor:in) / Elsner, Ronald (Autor:in) / Ramsey, Brian (Autor:in) / Wilson-Hodge, Colleen (Autor:in) / Tennant, Allyn (Autor:in) / Christe, Steven (Autor:in) / Shih, Albert (Autor:in) / Kiranmayee, Kilaru (Autor:in) / Swartz, Douglas (Autor:in) / Seller, Paul (Autor:in)

    Kongress:

    2015 IEEE Aerospace Conference ; 2015 ; Big Sky, MT, United States


    Erscheinungsdatum :

    2015-03-07


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch





    SuperHERO: Design of a new hard-X-ray focusing telescope

    Gaskin, Jessica / Elsner, Ronald / Ramsey, Brian et al. | IEEE | 2015


    SuperHERO: Next Generation Hard X-Ray Focusing Telescope

    Gaskin, J. / Wilson-Hodge, C. / Ramsey, B. et al. | NTRS | 2015



    SuperHERO: Design of a New Hard X-Ray Focusing Telescope

    Gaskin J. / Elsner R. / Wilson M. et al. | NTIS | 2015