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New models of Jupiter's magnetic field constrained by the Io flux tube footprint
DOI: 10.1029/97JA03726 Bibcode: 1998JGR...10311929C

Connerney, J. E. P.; Satoh, T.; Acuña, M. H. +1 more

Spherical harmonic models of the planetary magnetic field of Jupiter are obtained from in situ magnetic field measurements and remote observations of the position of the foot of the Io flux tube in Jupiter's ionosphere. The Io flux tube (IFT) footprint locates the ionospheric footprint of field lines traced from Io's orbital radial distance in the…

1998 Journal of Geophysical Research
eHST 341
Hubble Space Telescope imaging of Jupiter's UV aurora during the Galileo orbiter mission
DOI: 10.1029/98JE01130 Bibcode: 1998JGR...10320217C

Gérard, Jean-Claude; Clarke, John T.; Ben Jaffel, Lotfi

Hubble Space Telescope (HST) Wide-Field Planetary Camera 2 (WFPC 2) images of Jupiter's aurora have been obtained close in time with Galileo ultraviolet spectrometer (UVS) spectra and in situ particles, fields, and plasma wave measurements between June 1996 and July 1997, overlapping Galileo orbits G1, G2, G7, G8, and C9. This paper presents HST i…

1998 Journal of Geophysical Research
eHST 131
Detailed study of FUV Jovian auroral features with the post-COSTAR HST faint object camera
DOI: 10.1029/98JE01128 Bibcode: 1998JGR...10320195P

Prangé, Renée; Rego, Daniel; Pallier, Laurent +3 more

A set of Hubble Space Telescope faint object camera images taken in the H2 bands near 1550 Å is used to infer the morphological properties of the steady state Jovian FUV aurorae. We focus on issues best addressed using the excellent spatial resolution available after correction of the spherical aberration, i.e., those related to high la…

1998 Journal of Geophysical Research
eHST 97
Characteristics of the Galileo probe entry site from Earth-based remote sensing observations
DOI: 10.1029/98JE02380 Bibcode: 1998JGR...10322791O

Baines, Kevin H.; Hora, Joseph; Hinkley, Sasha +14 more

A reassessment of ground-based observations confirms to better than a 98% confidence level that the Galileo probe entered a 5-µm hot spot, a region of unusual clarity and dryness, some 900+/-300km north of its southern boundary. Cloud conditions at that point were similar to those in the center of this region, some 600 km further north. At t…

1998 Journal of Geophysical Research
eHST 83
OH in Saturn's magnetosphere: Observations and implications
DOI: 10.1029/98JE01127 Bibcode: 1998JGR...10320245R

Richardson, J. D.; McGrath, M. A.; Eviatar, A. +1 more

The discovery of OH in Saturn's inner magnetosphere changed our view of this region from one where plasma dominated the physics to one where neutrals are dominant. We revisit Hubble Space Telescope observations of OH and derive revised OH brightnesses for observations in 1992, 1994, and 1995. These OH observations as well as Voyager observations a…

1998 Journal of Geophysical Research
eHST 69
Saturn's hydrogen aurora: Wide field and planetary camera 2 imaging from the Hubble Space Telescope
DOI: 10.1029/98JE01324 Bibcode: 1998JGR...10320237T

Krist, John E.; Holtzman, Jon A.; Trauger, John T. +8 more

Wide field and planetary camera 2/Hubble Space Telescope (WFPC2/HST) images of Saturn's far ultraviolet aurora reveal emissions confined to a narrow band of latitudes near Saturn's north and south poles. The aurorae are most prominent in the morning sector with patterns that appear fixed in local time. The geographic distribution and vertical exte…

1998 Journal of Geophysical Research
eHST 38