A new particulate thermophysical model of the lunar soil is described which utilizes the results of laboratory experiments with evacuated powders. Excellent agreement is achieved with data acquired at far infrared and millimeter wavelengths. The parameters of the model are consistent with soil properties deduced from Surveyor spacecraft experiments. With minor modifications, the model may be useful in current efforts to interpret passive radiation from Mercury. (Author)


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    A New Thermophysical Model of the Lunar Soil


    Beteiligte:
    D. F. Winter (Autor:in) / J. M. Saari (Autor:in)

    Erscheinungsdatum :

    1968


    Format / Umfang :

    17 pages


    Medientyp :

    Report


    Format :

    Keine Angabe


    Sprache :

    Englisch





    Thermophysical property models for lunar regolith

    Schreiner, Samuel S | Online Contents | 2016


    Thermophysical property models for lunar regolith

    Schreiner, Samuel S | Online Contents | 2015


    Thermophysical properties of lunar volcanic deposits

    Glotch, Tim / Hayne, Paul O. / Elder, Catherine M. | NTRS | 2017


    Thermophysical properties of lunar red spots

    Glotch, T.D. / Hayne, P.O. / Elder, C.M. | NTRS | 2017