Geometrical considerations are presented for analyzing use of the stellar occultation technique on long-duration earth atmosphere monitoring missions. Simulated mission data are presented for three representative orbits. Bright near-IR stars are used as examples of how extensive global longitude-latitude coverage can be obtained by performing occultation measurements on several stars during the course of a 1-year mission. A brief comparison is made with similar missions using the sun as a light source.


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    Titel :

    The geometry of stellar occultation measurements on long-duration atmospheric monitoring missions


    Beteiligte:
    Brooks, D. R. (Autor:in)

    Kongress:

    American Astronautical Society and American Institute of Aeronautics and Astronautics, Astrodynamics Specialist Conference ; 1979 ; Provincetown, MA


    Erscheinungsdatum :

    01.06.1979


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


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