The Extreme Ultraviolet Explorer (EUVE) mission, currently scheduled from launch in September 1991, is described. The primary purpose of the mission is to survey the celestial sphere for astronomical sources of extreme ultraviolet (EUV) radiation with the use of three EUV telescope, each sensitive to a different segment of the EUV band. A fourth telescope is planned to perform a high-sensitivity search of a limited sample of the sky in the shortest wavelength bands. The all-sky survey is planned to be carried out in the first six months of the mission in four bands, or colors, 70-180 A, 170-250 A, 400-600 A, and 500-700 A. The second phase of the mission is devoted to spectroscopic observations of EUV sources. A high-efficiency grazing-incidence spectrometer using variable line-space gratings is planned to provide spectral data with about 1-A resolution. An end-to-end model of the mission, from a stellar source to the resulting scientific data, is presented. Hypothetical data from astronomical sources were processed through this model and are shown.


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    Titel :

    The Extreme Ultraviolet Explorer Mission


    Beteiligte:
    Bowyer, S. (Autor:in) / Malina, R. F. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1991-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    The Extreme Ultraviolet Explorer mission

    MALINA, R. / BATTEL, S. | AIAA | 1989


    The extreme ultraviolet explorer mission

    Bowyer, S. / Malina, R.F. | Elsevier | 1991


    The Extreme Ultraviolet Explorer mission - Overview and initial results

    Haisch, B. / Bowyer, S. / Malina, R. F. | NTRS | 1993


    The Extreme Ultraviolet Explorer mission - Instrumentation and science goals

    Bowyer, Stuart / Malina, Roger F. / Marshall, Herman L. | NTRS | 1988