References

[AJK+12]

B. J. Anderson, C. L. Johnson, H. Korth, R. M. Winslow, J. E. Borovsky, M. E. Purucker, J. A. Slavin, S. C. Solomon, M. T. Zuber, and R. L. McNutt Jr. Low-degree structure in mercury’s planetary magnetic field. Journal of Geophysical Research: Planets, 2012. doi:10.1029/2012JE004159.

[Bag94]

F. Bagenal. Empirical model of the io plasma torus: voyager measurements. Journal of Geophysical Research: Space Physics, 99(A6):11043–11062, 1994. doi:10.1029/93JA02908.

[BGB+17]

B. Bonfond, D. Grodent, S.V. Badman, J. Saur, J.-C. Gérard, and A. Radioti. Similarity of the jovian satellite footprints: spots multiplicity and dynamics. Icarus, 292:208–217, 2017. doi:10.1016/j.icarus.2017.01.009.

[BGG+09]

B. Bonfond, D. Grodent, J.-C. Gérard, A. Radioti, V. Dols, P. A. Delamere, and J. T. Clarke. The io uv footprint: location, inter-spot distances and tail vertical extent. Journal of Geophysical Research: Space Physics, 114(A7):, 2009. doi:10.1029/2009JA014312.

[Con92]

J. E. P. Connerney. Doing more with Jupiter’s magnetic field. In S. J. Bauer and H. O. Rucker, editors, Planetary Radio Emissions III, pages 13–33. Austria Acad. of Sci. Press, Vienna, 1992. URL: https://austriaca.at/?arp=0x0015cd0e.

[Con07]

J. E. P. Connerney. Planetary Magnetism. In Tilman Spohn, editor, Treatise on Geophysics: Planets and Moons, volume 10, pages 243–280. Elsevier, 2007.

[CAN81]

J. E. P. Connerney, M. H. Acuna, and N. F. Ness. Modeling the Jovian current sheet and inner magnetosphere. J. Geophys. Res., 86:8370–8384, 1981. doi:10.1029/JA086iA10p08370.

[CAN84]

J. E. P. Connerney, M. H. Acuna, and N. F. Ness. The Z3 Model of Saturn’s Magnetic Field and the Pioneer 11 Vector Helium Magnetometer Observations. J. Geophys. Res., 89:7541–7544, 1984. doi:10.1029/JA089iA09p07541.

[CAN87]

J. E. P. Connerney, M. H. Acuna, and N. F. Ness. The magnetic field of Uranus. J. Geophys. Res., 92:15329–15336, 1987. doi:10.1029/JA092iA13p15329.

[CANS98]

J. E. P. Connerney, M. H. Acuna, N. F. Ness, and T. Satoh. New Models of Jupiter’s Magnetic Field Constrained by the Io Flux Tube Footprint. J. Geophys. Res., 103:11929–11939, 1998. doi:10.1029/97JA03726.

[CKO+18]

J. E. P. Connerney, S. Kotsiaros, R. J. Oliversen, J. R. Espley, J. L. Joergensen, P. S. Joergensen, J. M. G. Merayo, and et al. A New Model of Jupiter’s Magnetic Field From Juno’s First Nine Orbits. Geophys. Res. Lett., 45:2590–2596, 2018. doi:10.1007/s11214-009-9621-7.

[CTHJ20]

J. E. P. Connerney, S. Timmins, M. Herceg, and J. L. Joergensen. A Jovian Magnetodisc Model for the Juno Era. Journal of Geophysical Research (Space Physics), 125(10):e28138, October 2020. doi:10.1029/2020JA028138.

[CTO+22]

J. E. P. Connerney, S. Timmins, R. J. Oliversen, J. R. Espley, J. L. Joergensen, S. Kotsiaros, P. S. Joergensen, J. M. G. Merayo, M. Herceg, J. Bloxham, K. M. Moore, A. Mura, A. Moirano, S. J. Bolton, and S. M. Levin. A New Model of Jupiter’s Magnetic Field at the Completion of Juno’s Prime Mission. Journal of Geophysical Research (Planets), 127(2):e07055, February 2022. doi:10.1029/2021JE007055.

[DS90]

Davis, L. Jr and E. Smith. A Model of Saturn’s Magnetic Field Based on All Available Data. J. Geophys. Res., 95:15257–15261, 1990. doi:10.1029/JA095iA09p15257.

[Her09]

F. Herbert. Aurora and magnetic field of uranus. J. Geophys. Res., 2009. doi:10.1029/2009JA014394.

[HBBL17]

S. L. G. Hess, B. Bonfond, F. Bagenal, and L. Lamy. A Model of the Jovian Internal Field Derived from in-situ and Auroral Constraints. In PRE8 Proceedings, volume 8. Austrian Academy of Science, 2017. doi:10.1553/PRE8s157.

[HBZG11]

S. L. G. Hess, B. Bonfond, P. Zarka, and D. Grodent. Model of the Jovian Magnetic Field Topology Constrained by the Io Auroral Emissions. J. Geophys. Res., 116:177, 2011. doi:10.1029/2010JA016262.

[HCZ08]

S. L. G. Hess, B. Cecconi, and P. Zarka. Modeling of Io-Jupiter Decameter Arcs, Emission Beaming and Energy Source. Geophys. Res. Lett., 2008. doi:10.1029/2008GL033656.

[HZ11]

S. L. G. Hess and P. Zarka. Modeling the radio signature of the orbital parameters, rotation, and magnetic field of exoplanets. Astronomy & Astrophysics, 531:A29, July 2011. doi:10.1051/0004-6361/201116510.

[HTK98]

D. P. Hinson, J. D. Twicken, and E. T. Karayel. Jupiter’s ionosphere: new results from voyager 2 radio occultation measurements. Journal of Geophysical Research: Space Physics, 103(A5):9505–9520, 1998. doi:10.1029/97JA03689.

[HBB19]

P. C. Hinton, F. Bagenal, and B. Bonfond. Alfvén wave propagation in the io plasma torus. Geophysical Research Letters, 46(3):1242–1249, 2019. doi:10.1029/2018GL081472.

[HGL+23]

V. Hue, G. R. Gladstone, C. K. Louis, T. K. Greathouse, B. Bonfond, J. R. Szalay, A. Moirano, R. S. Giles, J. A. Kammer, M. Imai, A. Mura, M. H. Versteeg, G. Clark, J. -C. Gérard, D. C. Grodent, J. Rabia, A. H. Sulaiman, S. J. Bolton, and J. E. P. Connerney. The Io, Europa, and Ganymede Auroral Footprints at Jupiter in the Ultraviolet: Positions and Equatorial Lead Angles. Journal of Geophysical Research (Space Physics), 128(5):e2023JA031363, May 2023. doi:10.1029/2023JA031363.

[LHC+19]

C. K. Louis, S. L. G. Hess, B. Cecconi, P. Zarka, L. Lamy, S. Aicardi, and A. Loh. ExPRES: an Exoplanetary and Planetary Radio Emissions Simulator. Astronomy and Astrophysics, 627:A30, 2019. doi:10.1051/0004-6361/201935161.

[LLZ+17a]

C. K. Louis, L. Lamy, P. Zarka, B. Cecconi, and S. L. G. Hess. Detection of Jupiter decametric emissions controlled by Europa and Ganymede with Voyager/PRA and Cassini/RPWS. J. geophys. Res. Space Physics, 122:1–20, September 2017. doi:10.1002/2016JA023779.

[LLZ+17b]

C. K. Louis, L. Lamy, P. Zarka, B. Cecconi, M. Imai, W. S. Kurth, G. Hospodarsky, S. L. G. Hess, X. Bonnin, S. J. Bolton, J. E. P. Connerney, and S. M. Levin. Io-Jupiter decametric arcs observed by Juno/Waves compared to ExPRES simulations. Geophys. Res. Lett., pages 1–17, 2017. doi:10.1002/2017GL073036.

[Wu85]

C.-W. Wu. Kinetic cyclotron and synchroton Maser instabilities: Radio emission processes by direct amplification of radiation. Space Sci. Rev., 41:215–298, 1985.

[ZLZ+25]

P. Zarka, C. K. Louis, J. Zhang, H. Tian, J. Morin, and Y. Gao. Location and energy of electrons producing the radio bursts from AD Leo observed by FAST in December 2021. \aap , 695:A95, March 2025. arXiv:2501.16180, doi:10.1051/0004-6361/202450950.