The measurement of inhomogeneities in the electron content along the orbital paths of Gemini 8 and Gemini 9 missions was not accomplished because the tracking information was not available. The use of ultrahigh frequency radio transmission was the primary factor in the successful removal of a very high frequency Faraday rotation ambiguity; but, as was expected, this was not very useful for fine-scale polarization studies. Ionosonde data were useful in the computation of the slab thickness at the closest point of approach of the spacecraft.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    Experiment Do14: Ultrahigh and very high frequency polarization


    Beteiligte:
    Ellis, R. E. (Autor:in)


    Erscheinungsdatum :

    01.09.1971


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Ultrahigh-speed polarization modulator

    Bull, J.D. / Kato, H. / Reid, A.R. et al. | IEEE | 2005


    Very high frequency radio

    Prendergast, L.J. | Engineering Index Backfile | 1946


    Very high frequency radio

    Prendergast, L.J. | Engineering Index Backfile | 1946


    Very high frequency radio

    Prendergast, L.J. | Engineering Index Backfile | 1946


    System design of the ultrahigh velocity GEDI experiment

    Laughlin, R.L. / Gully, J.H. / Nalty, K.E. et al. | Tema Archiv | 1986