Time-resolved observations of Jupiter's far-ultraviolet aurora

Gilda E. Ballester, John T. Clarke, John T. Trauger, Walter M. Harris, Karl R. Stapelfeldt, David Crisp, Robin W. Evans, Eric B. Burgh, Christopher J. Burrows, Stefano Casertano, John S. Gallagher, Richard E. Griffiths, J. Jeff Hester, John G. Hoessel, Jon A. Holtzman, John E. Krist, Vikki Meadows, Jeremy R. Mould, Raghvendra Sahai, Paul ScowenAlan M. Watson, James A. Westphal

Research output: Contribution to journalArticlepeer-review

74 Scopus citations

Abstract

Simultaneous imaging and spectroscopic observations of Jupiter's far- ultraviolet aurora covering half a jovian rotation were made on 31 May 1994. The Hubble Space Telescope Wide Field Planetary Camera 2 images revealed dramatic and rapidly changing auroral features, including discrete longitudinal structures along the auroral ovals, with variable contrast; a poleward offset in a north oval sector, showing equatorward motion near dusk; emissions polewards of the ovals, apparently co-rotating; and a bright event developing near the dawn limb. Viewing geometry effects explain the rotational intensity modulation observed by the International Ultraviolet Explorer, without intrinsic longitudinal asymmetries.

Original languageEnglish (US)
Pages (from-to)409-413
Number of pages5
JournalScience
Volume274
Issue number5286
DOIs
StatePublished - Oct 18 1996

ASJC Scopus subject areas

  • General

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