Abstract

The Juno spacecraft acquired direct observations of the jovian magnetosphere and auroral emissions from a vantage point above the poles. Juno's capture orbit spanned the jovian magnetosphere from bow shock to the planet, providing magnetic field, charged particle, and wave phenomena context for Juno's passage over the poles and traverse of Jupiter's hazardous inner radiation belts. Juno's energetic particle and plasma detectors measured electrons precipitating in the polar regions, exciting intense aurorae, observed simultaneously by the ultraviolet and infrared imaging spectrographs. Juno transited beneath the most intense parts of the radiation belts, passed about 4000 kilometers above the cloud tops at closest approach, well inside the jovian rings, and recorded the electrical signatures of high-velocity impacts with small particles as it traversed the equator.

Highlights

  • Charged particles travel in helical trajectories about the magnetic field

  • The Belgian contribution to UVS is enabled via support from the Belgian Science Policy Office (BELSPO) and the European Space Agency’s Program de Development d’Experiences Scientifiques (PRODEX)

  • The Juno mission is part of the New Frontiers Program managed at NASA's Marshall Space Flight Center in Huntsville, Alabama

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Summary

Introduction

J. Bolton et al, Science 356, 821–825 (2017). J. McComas et al, Space Sci. Rev. R. Gladstone et al, Space Sci. Rev. A. Balogh et al, Science 257, 1515–1518 (1992).

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