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Control of Jupiter's radio emission and aurorae by the solar wind
DOI: 10.1038/415985a Bibcode: 2002Natur.415..985G

Gurnett, D. A.; Persoon, A. M.; Dougherty, M. K. +14 more

Radio emissions from Jupiter provided the first evidence that this giant planet has a strong magnetic field and a large magnetosphere. Jupiter also has polar aurorae, which are similar in many respects to Earth's aurorae. The radio emissions are believed to be generated along the high-latitude magnetic field lines by the same electrons that produc…

2002 Nature
Cassini 131
Ultra-relativistic electrons in Jupiter's radiation belts
DOI: 10.1038/415987a Bibcode: 2002Natur.415..987B

Johnson, W. T. K.; Klein, M.; Hofstadter, M. +18 more

Ground-based observations have shown that Jupiter is a two-component source of microwave radio emission: thermal atmospheric emission and synchrotron emission from energetic electrons spiralling in Jupiter's magnetic field. Later in situ measurements confirmed the existence of Jupiter's high-energy electron-radiation belts, with evidence for elect…

2002 Nature
Cassini 102
The dusk flank of Jupiter's magnetosphere
DOI: 10.1038/415991a Bibcode: 2002Natur.415..991K

Gurnett, D. A.; Dougherty, M. K.; Hospodarsky, G. B. +8 more

Limited single-spacecraft observations of Jupiter's magnetopause have been used to infer that the boundary moves inward or outward in response to variations in the dynamic pressure of the solar wind. At Earth, multiple-spacecraft observations have been implemented to understand the physics of how this motion occurs, because they can provide a snap…

2002 Nature
Cassini 38
Planetary science: Magnetic moments at Jupiter
DOI: 10.1038/415965a Bibcode: 2002Natur.415..965H

Hill, Thomas W.

The coming together of two spacecraft near Jupiter provided a unique opportunity to investigate the giant planet's magnetic field -- and the results, collected in this issues, are stunning

2002 Nature
Cassini 8