Abstract Solar radio emissions at long wavelengths (wavelengths greater than 10 m or frequencies smaller than 30 MHz) are produced in the upper corona and in the interplanetary medium (the Heliosphere), sometimes at very large distances from the Sun, up to the orbit of Jupiter and beyond. Solar radio emissions are produced by the passage of energetic particles and shock waves; they provide a unique means to detect perturbations originating from the solar activity and to track their progression through the interplanetary medium. Different aspects of current research are presented, essentially based on results of the URAP investigation on ULYSSES.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Radio waves in the heliosphere


    Beteiligte:

    Erschienen in:

    Advances in Space Research ; 13 , 6 ; 191-203


    Erscheinungsdatum :

    01.01.1993


    Format / Umfang :

    13 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    Radio Waves in the Heliosphere

    Bougeret, J.-L. | Online Contents | 1993


    Radio Emissions in the Heliosphere

    Bougeret, J. L. / COSPAR / Scientific Committee on Solar Terrestrial Physics | British Library Conference Proceedings | 1995


    Radio Emissions in the Heliosphere

    Bougeret, J.L. | Online Contents | 1995



    Magnetic fields throughout the heliosphere

    Smith, Edward J. | NTRS | 1993