In order to make astronomical observations from the Shuttle, the observer needs good information on the intensities and spectral characteristics of various sources. This paper presents a model spectrum for the natural airglow background. The spectrum is modeled over a wavelength range extending from the extreme ultraviolet to the near-infrared. This model is based on the present knowledge of the upper atmosphere. The effect of different viewing configurations is illustrated, together with day-to-night variations. The results synthesized here assume an ideal vehicle in the sense that no contaminant emissions are induced by the Shuttle and payload. These spectra therefore represent a baseline which can be used to locate unanticipated or nonambient features.


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    Titel :

    The natural background at Shuttle altitudes


    Beteiligte:
    Torr, Marsha R. (Autor:in) / Owens, J. K. (Autor:in) / Eun, J. W. (Autor:in) / Torr, D. G. (Autor:in) / Richards, P. G. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.01.1987



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    The natural background at shuttle altitudes

    Torr, Marsha R. / Owens, J.K. / Eun, J.W. et al. | Elsevier | 1987


    Aerodynamics of Shuttle Orbiter at High Altitudes

    Rault, D. F. G. / AIAA | British Library Conference Proceedings | 1993


    Aerodynamics of Shuttle Orbiter at high altitudes

    Rault, Didier F. G. | NTRS | 1993



    Aerodynamics of the Shuttle Orbiter at High Altitudes

    Rault, D.F.G. | Online Contents | 1994