Simultaneous X-ray, Ultraviolet, and Radio Observations of Jupiter's Aurora

Details Simultaneous X-ray, Ultraviolet, and Radio Observations of Jupiter's Aurora Simultaneous X-ray, Ultraviolet, and Radio Observations of Jupiter's Aurora

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agusmsh21b..02w&link_type=abstract

American Geophysical Union, Spring Meeting 2004, abstract #SH21B-02

Physics

2704 Auroral Phenomena (2407), 2708 Current Systems (2409), 2784 Solar Wind/Magnetosphere Interactions

Scientific paper

Chandra observations of 40-minute periodicity in X-ray emissions from Jupiter's polar caps during the Cassini-Huygens 2000 Jupiter flyby are reminiscent of the correlation in a near-40-minute periodicity between quasi-periodic radio bursts and energetic field-aligned electron flows on Jupiter's dusk flank as measured by the Ulysses spacecraft in its initial Jupiter flyby. Follow-up observations using both Chandra and Ulysses are inconclusive, but simultaneous HST observations and X-ray spectral data provide tantalizing clues of a possible mechanism.

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