29 citations as recorded by crossref.

1. Jupiter’s Magnetosphere: Plasma Sources and Transport S. Bolton et al. 10.1007/s11214-015-0184-5
2. Comment on “Jupiter: A fundamentally different magnetospheric interaction with the solar wind” by D. J. McComas and F. Bagenal S. Cowley et al. 10.1029/2007GL032645
3. How does the Sun Influence the Magnetospheres of Jupiter and Saturn? C. Jackman & C. Arridge 10.1017/S1743921317011620
4. How Jupiter’s unusual magnetospheric topology structures its aurora B. Zhang et al. 10.1126/sciadv.abd1204
5. Characteristics of solar wind control on Jovian UV auroral activity deciphered by long‐term Hisaki EXCEED observations: Evidence of preconditioning of the magnetosphere? H. Kita et al. 10.1002/2016GL069481
6. Solar Cycle Effects on the Dynamics of Jupiter’s and Saturn’s Magnetospheres C. Jackman & C. Arridge 10.1007/s11207-011-9748-z
7. Response of Jupiter's auroras to conditions in the interplanetary medium as measured by the Hubble Space Telescope and Juno J. Nichols et al. 10.1002/2017GL073029
8. Global MHD simulations of the Response of Jupiter's Magnetosphere and Ionosphere to Changes in the Solar Wind and IMF Y. Sarkango et al. 10.1029/2019JA026787
9. A Review of General Physical and Chemical Processes Related to Plasma Sources and Losses for Solar System Magnetospheres K. Seki et al. 10.1007/s11214-015-0170-y
10. Large-Scale Structure and Dynamics of the Magnetotails of Mercury, Earth, Jupiter and Saturn C. Jackman et al. 10.1007/s11214-014-0060-8
11. Jupiter's Dark Polar Region as Observed by the Hubble Space Telescope During the Juno Approach Phase B. Swithenbank‐Harris et al. 10.1029/2019JA027306
12. Magnetodisc modelling in Jupiter's magnetosphere using Juno magnetic field data and the paraboloid magnetic field model I. Pensionerov et al. 10.5194/angeo-37-101-2019
13. Magnetosonic Mach number dependence of the efficiency of reconnection between planetary and interplanetary magnetic fields A. Grocott et al. 10.1029/2009JA014330
14. Magnetospheric Science Objectives of the Juno Mission F. Bagenal et al. 10.1007/s11214-014-0036-8
15. Magnetosphere-ionosphere coupling at Jupiter-like exoplanets with internal plasma sources: implications for detectability of auroral radio emissions J. Nichols 10.1111/j.1365-2966.2011.18528.x
16. In situ evidence of the magnetospheric cusp of Jupiter from Juno spacecraft measurements Y. Xu et al. 10.1038/s41467-024-50449-z
17. Variation of different components of Jupiter's auroral emission J. Nichols et al. 10.1029/2009JA014051
18. Review of Mercury’s dynamic magnetosphere: Post-MESSENGER era and comparative magnetospheres W. Sun et al. 10.1007/s11430-021-9828-0
19. Response of Jupiter's UV auroras to interplanetary conditions as observed by the Hubble Space Telescope during the Cassini flyby campaign J. Nichols et al. 10.1029/2006JA012005
20. Magnetic flux circulation in the rotationally driven giant magnetospheres P. Delamere et al. 10.1002/2015JA021036
21. Magnetic Reconnection at Planetary Bodies and Astrospheres D. Gershman et al. 10.1007/s11214-023-01017-2
22. Saturn's dayside ultraviolet auroras: Evidence for morphological dependence on the direction of the upstream interplanetary magnetic field C. Meredith et al. 10.1002/2013JA019598
23. In-Situ Observations of Reconnection in Space G. Paschmann et al. 10.1007/s11214-012-9957-2
24. Structure and statistical properties of plasmoids in Jupiter's magnetotail M. Vogt et al. 10.1002/2013JA019393
25. Observations of Jovian polar auroral filaments J. Nichols et al. 10.1029/2009GL037578
26. Using in situ solar-wind observations to generate inner-boundary conditions to outer-heliosphere simulations – I. Dynamic time warping applied to synthetic observations M. Owens & J. Nichols 10.1093/mnras/stab2512
27. Solar Wind and Internally Driven Dynamics: Influences on Magnetodiscs and Auroral Responses P. Delamere et al. 10.1007/s11214-014-0075-1
28. Long‐Term Variability of Jupiter's Magnetodisk and Implications for the Aurora M. Vogt et al. 10.1002/2017JA024066
29. Planetary space weather: scientific aspects and future perspectives C. Plainaki et al. 10.1051/swsc/2016024