Far-ultraviolet imaging of Jupiter's aurora and the Io 'footprint'

John T. Clarke; Gilda E. Ballester; John Trauger; Robin Evans; J. E.P. Connerney; Karl Stapelfeldt; David Crisp; Paul D. Feldman; 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; Paul A. Scowen; Alan M. Watson; James A. Westphal

doi:10.1126/science.274.5286.404

Far-ultraviolet imaging of Jupiter's aurora and the Io 'footprint'

John T. Clarke, Gilda E. Ballester, John Trauger, Robin Evans, J. E.P. Connerney, Karl Stapelfeldt, David Crisp, Paul D. Feldman, 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, Paul A. Scowen, Alan M. WatsonJames A. Westphal

Research output: Contribution to journal › Article › peer-review

189 Scopus citations

Abstract

Far-ultraviolet images of Jupiter from the Hubble Space Telescope Wide Field Planetary Camera 2 reveal polar auroral emissions at 300 kilometer resolution and three times higher sensitivity than previously achieved. Persistent features include a main oval containing most of the emission and magnetically connected to the middle magnetosphere, diffuse and variable emissions poleward of the main oval, and discrete emission from Io's magnetic footprint equatorward of the oval. The auroral emissions are variable, exhibit magnetic conjugacy, and are visible above the planet limb. All emissions approximately co-rotate with Jupiter except the Io 'footprint,' which is fixed along Io's magnetic flux tube.

Original language	English (US)
Pages (from-to)	404-409
Number of pages	6
Journal	Science
Volume	274
Issue number	5286
DOIs	https://doi.org/10.1126/science.274.5286.404
State	Published - Oct 18 1996
Externally published	Yes

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Clarke, J. T., Ballester, G. E., Trauger, J., Evans, R., Connerney, J. E. P., Stapelfeldt, K., Crisp, D., Feldman, P. D., 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., Scowen, P. A., ... Westphal, J. A. (1996). Far-ultraviolet imaging of Jupiter's aurora and the Io 'footprint'. Science, 274(5286), 404-409. https://doi.org/10.1126/science.274.5286.404

Clarke, JT, Ballester, GE, Trauger, J, Evans, R, Connerney, JEP, Stapelfeldt, K, Crisp, D, Feldman, PD, Burrows, CJ, Casertano, S, Gallagher, JS, Griffiths, RE, Hester, JJ, Hoessel, JG, Holtzman, JA, Krist, JE, Meadows, V, Mould, JR, Scowen, PA, Watson, AM & Westphal, JA 1996, 'Far-ultraviolet imaging of Jupiter's aurora and the Io 'footprint'', Science, vol. 274, no. 5286, pp. 404-409. https://doi.org/10.1126/science.274.5286.404

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title = "Far-ultraviolet imaging of Jupiter's aurora and the Io 'footprint'",

abstract = "Far-ultraviolet images of Jupiter from the Hubble Space Telescope Wide Field Planetary Camera 2 reveal polar auroral emissions at 300 kilometer resolution and three times higher sensitivity than previously achieved. Persistent features include a main oval containing most of the emission and magnetically connected to the middle magnetosphere, diffuse and variable emissions poleward of the main oval, and discrete emission from Io's magnetic footprint equatorward of the oval. The auroral emissions are variable, exhibit magnetic conjugacy, and are visible above the planet limb. All emissions approximately co-rotate with Jupiter except the Io 'footprint,' which is fixed along Io's magnetic flux tube.",

author = "Clarke, {John T.} and Ballester, {Gilda E.} and John Trauger and Robin Evans and Connerney, {J. E.P.} and Karl Stapelfeldt and David Crisp and Feldman, {Paul D.} 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 Scowen, {Paul A.} and Watson, {Alan M.} and Westphal, {James A.}",

year = "1996",

month = oct,

day = "18",

doi = "10.1126/science.274.5286.404",

language = "English (US)",

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T1 - Far-ultraviolet imaging of Jupiter's aurora and the Io 'footprint'

AU - Clarke, John T.

AU - Ballester, Gilda E.

AU - Trauger, John

AU - Evans, Robin

AU - Connerney, J. E.P.

AU - Stapelfeldt, Karl

AU - Crisp, David

AU - Feldman, Paul D.

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 - Scowen, Paul A.

AU - Watson, Alan M.

AU - Westphal, James A.

PY - 1996/10/18

Y1 - 1996/10/18

N2 - Far-ultraviolet images of Jupiter from the Hubble Space Telescope Wide Field Planetary Camera 2 reveal polar auroral emissions at 300 kilometer resolution and three times higher sensitivity than previously achieved. Persistent features include a main oval containing most of the emission and magnetically connected to the middle magnetosphere, diffuse and variable emissions poleward of the main oval, and discrete emission from Io's magnetic footprint equatorward of the oval. The auroral emissions are variable, exhibit magnetic conjugacy, and are visible above the planet limb. All emissions approximately co-rotate with Jupiter except the Io 'footprint,' which is fixed along Io's magnetic flux tube.

AB - Far-ultraviolet images of Jupiter from the Hubble Space Telescope Wide Field Planetary Camera 2 reveal polar auroral emissions at 300 kilometer resolution and three times higher sensitivity than previously achieved. Persistent features include a main oval containing most of the emission and magnetically connected to the middle magnetosphere, diffuse and variable emissions poleward of the main oval, and discrete emission from Io's magnetic footprint equatorward of the oval. The auroral emissions are variable, exhibit magnetic conjugacy, and are visible above the planet limb. All emissions approximately co-rotate with Jupiter except the Io 'footprint,' which is fixed along Io's magnetic flux tube.

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Far-ultraviolet imaging of Jupiter's aurora and the Io 'footprint'

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