Citation:
Wang, Y. M., Jia, X. Z., Wang, C. B., Wang, S., and Krupar, V. (2020). Locating the source field lines of Jovian decametric radio emissions. Earth Planet. Phys., 4(2), 95–104doi: 10.26464/epp2020015
2020, 4(2): 95-104. doi: 10.26464/epp2020015
Locating the source field lines of Jovian decametric radio emissions
| 1. | Chinese Academy of Sciences Key Laboratory of Geospace Environment, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China |
| 2. | Chinese Academy of Sciences Center for Excellence in Comparative Planetology, University of Science and Technology of China, Hefei 230026, China |
| 3. | Mengcheng National Geophysical Observatory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China |
| 4. | Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109-2143, USA |
| 5. | Universities Space Research Association, Columbia, Maryland, USA |
| 6. | NASA Goddard Space Flight Center, Greenbelt, Maryland, USA |
| 7. | Department of Space Physics, Institute of Atmospheric Physics, The Czech Academy of Sciences, Prague, Czech Republic |
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
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