Observations of radio emissions in the frequency range of 2 to 3 kHz have been made in the distant heliosphere by the Voyager 1 and 2 plasma wave instruments. Based primarily on wideband observations made periodically throughout the cruise phases of the missions the radio emission, first observed in 1982, appears to have been present almost continuously since 1983. The spectrum is complex, usually showing two peaks, one near 2 and another near 3 kHz. Occasionally, only one of the peaks is observed. A possible source for the radio emissions is the terminal shock in the outer heliosphere.


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    Titel :

    Recent observations of the very low frequency interplanetary radio emission


    Beteiligte:
    Kurth, W. S. (Autor:in) / Gurnett, D. A. (Autor:in) / Scarf, F. L. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.01.1986



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Recent observations of the very low frequency interplanetary radio emission

    Kurth, W.S. / Gurnett, D.A. / Scarf, F.L. | Elsevier | 1986


    Radio-scintillation observations of interplanetary disturbances

    Watanabe, Takashi / Kakinuma, Takakiyo | Elsevier | 1984




    Very high frequency radio

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