Now showing items 6-9 of 9

    • Ground support of Juno mission and RFI mitigation 

      Zakharenko, V.; Kharlanova, V.; Ryabov, V.; Yerin, S.; Brazhenko, A.; Fransuzenko, A.; Konovalenko, O. (2023)
      Joint observations provide much more useful data and improve the quality of the analysis. But to obtain high-quality results, it is often necessary to improve the algorithms of the processing program. Radio frequency ...
    • Jupiter Long Dispersion Lightning Whistlers that propagate through the Io torus: Juno Observations 

      Hospodarsky, G. B.; Milne, A. J.; Kurth, W. S.; Imai, M.; Kolmasová, I.; Santolík, O.; Connerney, J. E. P.; Bolton, S. J. (2023)
      The detection of lightning whistlers in planetary magnetospheres can provide valuable information about the properties of both the source lightning, and the plasma environment along the whistler propagation path. The Juno ...
    • Localisation of the main HOM source in the dusk side of the Jovian magnetosphere 

      Boudouma, A.; Zarka, P.; Magalhães, F. P.; Marques, M. S.; Louis, C. K.; Echer, E.; Lamy, L.; Prangé R. (2023)
      It was suggested in Zarka et al. (2021) that the most intense Jovian hectometric emissions (HOM) originate from the dusk side of the Jovian magnetosphere. These authors showed that the distribution of the main HOM observed ...
    • Probing Jupiter-satellite interactions from the beaming of their decametric emissions: the case of Europa and Ganymede 

      Lamy, L.; Duchêne, A.; Mauduit, E.; Zarka, P.; Yerin, S.; Louis, C.; Griessmeier, J.-M.; Girard, J.; Theureau, G. (2023)
      In a recent study, we accurately measured the beaming of Io-Jupiter decametric emissions, whose uncertainty is controlled by that on the position of the active Io ux tube (IFT) hosting the radiosources. The active IFT was ...