19 citations as recorded by crossref.

1. Jupiter's Double‐Arc Aurora as a Signature of Magnetic Reconnection: Simultaneous Observations From HST and Juno R. Guo et al.
2. Acceleration of Ions in Jovian Plasmoids: Does Turbulence Play a Role? E. Kronberg et al.
3. A Survey of Magnetic Field Line Curvature in Jovian Dawn Magnetodisc W. Gu et al.
4. Transient internally driven aurora at Jupiter discovered by Hisaki and the Hubble Space Telescope T. Kimura et al.
5. On the Relation Between Jovian Aurorae and the Loading/Unloading of the Magnetic Flux: Simultaneous Measurements From Juno, Hubble Space Telescope, and Hisaki Z. Yao et al.
6. Energetic particle evidence for magnetic filaments in Jupiter's magnetotail M. Hill et al.
7. Wavelet analysis of low frequency magnetic field fluctuations in the Jupiter’s magnetotail M. de Souza Echer et al.
8. Acceleration of ions in the Jupiter magnetotail: Particle resonant interaction with dipolarization fronts A. Artemyev et al.
9. Field-aligned beams and reconnection in the jovian magnetotail E. Kronberg et al.
10. Variation of Jupiter's Aurora Observed by Hisaki/EXCEED: 4. Quasi‐Periodic Variation C. Tao et al.
11. Magnetotail Reconnection at Jupiter: A Survey of Juno Magnetic Field Observations M. Vogt et al.
12. Thin current sheets in the Jovian magnetotail A. Artemyev et al.
13. Magnetic reconnection in the magnetodisk of centrifugally dominated giant planets R. Guo & Z. Yao
14. Hourly Periodic Variations of Ultralow‐Frequency (ULF) Waves in Jupiter's Magnetosheath W. Gu et al.
15. Reconnection and flows in the Jovian magnetotail as inferred from magnetometer observations M. Vogt et al.
16. Magnetic Reconnection and Associated Transient Phenomena Within the Magnetospheres of Jupiter and Saturn P. Louarn et al.
17. Structure and statistical properties of plasmoids in Jupiter's magnetotail M. Vogt et al.
18. Jovian deep magnetotail composition and structure D. McComas et al.
19. Solar Wind Interaction With Jupiter's Magnetosphere: A Statistical Study of Galileo In Situ Data and Modeled Upstream Solar Wind Conditions M. Vogt et al.