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 A. Scowen; Alan M. Watson; James A. Westphal

doi:10.1126/science.274.5286.409

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 A. Scowen

Alan M. Watson, James A. Westphal

Research output: Contribution to journal › Article › peer-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 language	English (US)
Pages (from-to)	409-413
Number of pages	5
Journal	Science
Volume	274
Issue number	5286
DOIs	https://doi.org/10.1126/science.274.5286.409
State	Published - Oct 18 1996
Externally published	Yes

ASJC Scopus subject areas

General

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Cite this

Ballester, G. E., Clarke, J. T., Trauger, J. T., Harris, W. M., Stapelfeldt, K. R., Crisp, D., Evans, R. W., Burgh, E. B., Burrows, C. J., Casertano, S., Gallagher, J. S., Griffiths, R. E., Hester, J. J., Hoessel, J. G., Holtzman, J. A., Krist, J. E., Meadows, V., Mould, J. R., Sahai, R., ... Westphal, J. A. (1996). Time-resolved observations of Jupiter's far-ultraviolet aurora. Science, 274(5286), 409-413. https://doi.org/10.1126/science.274.5286.409

Ballester, GE, Clarke, JT, Trauger, JT, Harris, WM, Stapelfeldt, KR, Crisp, D, Evans, RW, Burgh, EB, Burrows, CJ, Casertano, S, Gallagher, JS, Griffiths, RE, Hester, JJ, Hoessel, JG, Holtzman, JA, Krist, JE, Meadows, V, Mould, JR, Sahai, R, Scowen, PA, Watson, AM & Westphal, JA 1996, 'Time-resolved observations of Jupiter's far-ultraviolet aurora', Science, vol. 274, no. 5286, pp. 409-413. https://doi.org/10.1126/science.274.5286.409

@article{d9dad0365666477b9223fbd917a126b9,

title = "Time-resolved observations of Jupiter's far-ultraviolet aurora",

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.",

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

year = "1996",

month = oct,

day = "18",

doi = "10.1126/science.274.5286.409",

language = "English (US)",

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pages = "409--413",

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publisher = "American Association for the Advancement of Science",

number = "5286",

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TY - JOUR

T1 - Time-resolved observations of Jupiter's far-ultraviolet aurora

AU - Ballester, Gilda E.

AU - Clarke, John T.

AU - Trauger, John T.

AU - Harris, Walter M.

AU - Stapelfeldt, Karl R.

AU - Crisp, David

AU - Evans, Robin W.

AU - Burgh, Eric B.

AU - Burrows, Christopher J.

AU - Casertano, Stefano

AU - Gallagher, John S.

AU - Griffiths, Richard E.

AU - Hester, J. Jeff

AU - Hoessel, John G.

AU - Holtzman, Jon A.

AU - Krist, John E.

AU - Meadows, Vikki

AU - Mould, Jeremy R.

AU - Sahai, Raghvendra

AU - Scowen, Paul A.

AU - Watson, Alan M.

AU - Westphal, James A.

PY - 1996/10/18

Y1 - 1996/10/18

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/0012663823

UR - https://www.scopus.com/pages/publications/0012663823#tab=citedBy

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SN - 0036-8075

VL - 274

SP - 409

EP - 413

JO - Science

JF - Science

IS - 5286

ER -

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

Abstract

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