Locating the Source Field Lines of Jovian Decametric Radio Emissions

0523142 - ÚFA 2021 RIV CN eng J - Článek v odborném periodiku
Wang, Y. - Jia, X. - Wang, Ch. - Wang, S. - Krupař, Vratislav
Locating the Source Field Lines of Jovian Decametric Radio Emissions.
Earth and Planetary Physics. Roč. 4, č. 2 (2020), s. 95-104. ISSN 2096-3955
Grant CEP: GA ČR(CZ) GJ17-06818Y
Institucionální podpora: RVO:68378289
Klíčová slova: radio decametric emissions * Jovian magnetosphere * energetic electrons
Obor OECD: Fluids and plasma physics (including surface physics)
Způsob publikování: Open access
https://doi.org/10.26464/epp2020015

Decametric (DAM) radio emissions are one of the main windows through which one can reveal and understand the Jovian magnetospheric dynamics and its interaction with the moons. DAMs are generated by energetic electrons through cyclotron-maser instability. For Io (the most active moon) related DAMs, the energetic electrons are sourced from Io volcanic activities, and quickly trapped by neighboring Jovian magnetic field. To properly interpret the physical processes behind DAMs, it is important to precisely locate the source field lines from which DAMs are emitted. Following the work by Hess et al. [2008, 2010], we develop a method to locate the source region as well as the associated field lines for any given DAM emission recorded in a radio dynamic spectrum by, e.g., Wind/WAVES or STEREO/WAVES. The field lines are calculated by the state-of-art analytical model, called JRM09 [Connerney et al., 2018]. By using this method, we may also derive the emission cone angle and the energy of associated electrons. If multiple radio instruments at different perspectives saw the same DAM event, the evolution of its source region and associated field lines is able to be revealed. We apply the method to an Io-DAM event, and find that the method is valid and reliable. Some physical processes behind the DAM event are also discussed.
Trvalý link: http://hdl.handle.net/11104/0307536