IRAS sky survey measurements are used to constrain a model for the interplanetary dust emission. Efforts to date, although hampered somewhat by calibration uncertainties, indicate that the cloud is inclined to the ecliptic by approximately 1.7 deg, with its line of ascending nodes at 70 deg ecliptic longitude. The data is well fit by a dust density distribution presently described in cloud symmetry plane coordinates, where the dust has a gray emissivity and an equilibrium temperature at 1 AU of 280 K.


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    Titel :

    IRAS observations of the zodiacal background


    Beteiligte:
    Good, J. C. (Autor:in) / Gautier, T. N. (Autor:in) / Hauser, M. G. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.01.1986



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    IRAS observations of the zodiacal background

    Good, J.C. / Hauser, M.G. / Gautier, T.N. | Elsevier | 1987



    Space observations of the zodiacal light

    Weinberg, J. L. | NTRS | 1976


    OSO-B2 satellite observations of zodiacal light.

    Ney, E. P. / Sparrow, J. G. | NTRS | 1968


    Analysis of All Available Zodiacal Light Observations Final Report

    M. A. Alexander / R. R. Circle / A. G. Konheim et al. | NTIS | 1967