Observations from earth orbit and variability of the polar aurora on Jupiter

Astronomy and Astrophysics – Astronomy

Scientific paper

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Auroral Spectroscopy, Jupiter Atmosphere, Planetary Magnetic Fields, Polar Regions, Spaceborne Astronomy, Earth Orbits, Explorer Satellites, H Alpha Line, Planetary Magnetospheres, Ultraviolet Astronomy

Scientific paper

Spatially resolved spectra of Jupiter taken with the International Ultraviolet Explorer satellite show enhanced emissions from the polar regions at H L-alpha (1216 A) and in the Lyman and Werner bands of H2 (1175-1650 A). Two types of variability in emission brightness have been observed in these aurorae: an increase in the observed emission as the auroral oval rotates with Jupiter's magnetic pole to face toward the earth and a general variation in brightness of more than an order of magnitude under nearly identical observing conditions. In addition, the spectral character of these aurorae (determined by the ratio of H L-alpha to H2 brightnesses) appears variable, indicating that the depth of penetration of the auroral particles is not constant.

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