Search Publications

An investigation of Titan's aerosols using microwave analog measurements and radiative transfer modeling
DOI: 10.1016/j.icarus.2005.06.017 Bibcode: 2005Icar..179..511T

Kolokolova, L.; Gustafson, B. Å. S.; Thomas-Osip, J. E. +1 more

A combination of laboratory experiments, theoretical modeling, and spacecraft observations is employed to characterize the aerosols in the atmosphere of Titan. The scattering properties of model aerosols were measured using the Microwave Analog Light Scattering Facility at the University of Florida and complemented with theoretical modeling of sin…

2005 Icarus
Huygens 6
Keck infrared observations of Saturn's main rings bracketing Earth's August 1995 ring plane crossing
DOI: 10.1016/j.icarus.2004.10.008 Bibcode: 2005Icar..174..241V

de Pater, Imke; Showalter, Mark R.; Lissauer, Jack J. +1 more

We present results of near-infrared (2.26 µm) observations of Saturn's main rings taken with the W.M. Keck telescope during August 8-11, 1995, surrounding the time that Earth crossed Saturn's ring plane. These observations provide a unique opportunity to study the evolution of the ring brightness in detail, and by combining our data with Hub…

2005 Icarus
eHST 2
A search for temporal variability in the surface chemistry of the icy Galilean satellites
DOI: 10.1016/j.icarus.2004.10.005 Bibcode: 2005Icar..173...50D

Hendrix, Amanda; Domingue, Deborah

The purpose of this study was to determine if any temporal variability in the broadband UV spectral properties of the icy Galilean satellites exists, and if so, to characterize its spatial distribution as a function of longitude in order to attempt to correlate any temporal changes with satellite surface interactions with the space environment. Th…

2005 Icarus
IUE 2
New perspectives on Titan's upper atmosphere from a reanalysis of the Voyager 1 UVS solar occultations
DOI: 10.1016/j.icarus.2004.03.005 Bibcode: 2004Icar..170...91V

Strobel, Darrell F.; Vervack, Ronald J.; Sandel, Bill R.

We have reanalyzed the Voyager 1 UVS solar occultations by Titan to expand upon previous analyses and to resolve inconsistencies that have been noted in the scientific literature. To do so, we have developed a detailed model of the UVS detector and improved both the data reduction methods and retrieval techniques. In comparison to the values previ…

2004 Icarus
Huygens 136
Comet nucleus size distributions from HST and Keck telescopes
DOI: 10.1016/j.icarus.2004.03.014 Bibcode: 2004Icar..170..463M

Marsden, B. G.; Meech, K. J.; Hainaut, O. R.

The Wide Field Camera (WFC) on the Hubble Space Telescope and the Low Resolution Imaging Spectrograph (LRIS) on the Keck II telescope have been used to image 21 distant dynamically new, long-period (LP) and short-period (SP) Jupiter-family (JF) comet nuclei (near aphelion), as part of a long-term program to search for physical differences between …

2004 Icarus
eHST 125
Cassini UVIS observations of the Io plasma torus. I. Initial results
DOI: 10.1016/j.icarus.2003.12.027 Bibcode: 2004Icar..172...78S

Steffl, Andrew J.; Stewart, A. Ian F.; Bagenal, Fran

During the Cassini spacecraft's flyby of Jupiter (October, 2000-March, 2001), the Ultraviolet Imaging Spectrograph (UVIS) produced an extensive dataset consisting of 3349 spectrally dispersed images of the Io plasma torus. Here we present an example of the raw data and representative EUV spectra (561-1181 Å) of the torus, obtained on October 1, 20…

2004 Icarus
Cassini 84
Cassini UVIS observations of the Io plasma torus. II. Radial variations
DOI: 10.1016/j.icarus.2004.04.016 Bibcode: 2004Icar..172...91S

Steffl, Andrew J.; Stewart, A. Ian F.; Bagenal, Fran

On January 14, 2001, shortly after the Cassini spacecraft's closest approach to Jupiter, the Ultraviolet Imaging Spectrometer (UVIS) made a radial scan through the midnight sector of Io plasma torus. The Io torus has not been previously observed at this local time. The UVIS data consist of 2-D spectrally dispersed images of the Io plasma torus in …

2004 Icarus
Cassini 73
Cassini VIMS observations of the Galilean satellites including the VIMS calibration procedure
DOI: 10.1016/j.icarus.2004.07.001 Bibcode: 2004Icar..172..104M

Sotin, C.; Brown, R. H.; Baines, K. H. +22 more

The Visual and Infrared Mapping Spectrometer (VIMS) observed the Galilean satellites during the Cassini spacecraft's 2000/2001 flyby of Jupiter, providing compositional and thermal information about their surfaces. The Cassini spacecraft approached the jovian system no closer than about 126 Jupiter radii, about 9 million kilometers, at a phase ang…

2004 Icarus
Cassini 72
Retrievals of jovian tropospheric phosphine from Cassini/CIRS
DOI: 10.1016/j.icarus.2003.09.027 Bibcode: 2004Icar..172...37I

Irwin, P. G. J.; Calcutt, S. B.; Taylor, F. W. +4 more

On December 30th, 2000, the Cassini-Huygens spacecraft reached the perijove milestone on its continuing journey to the Saturnian System. During an extended six-month encounter, the Composite Infrared Spectrometer (CIRS) returned spectra of the jovian atmosphere, rings and satellites from 10-1400 cm -1 (1000-7 µm) at a programmable…

2004 Icarus
Cassini 69
The atmospheric signature of Io's Prometheus plume and anti-jovian hemisphere: evidence for a sublimation atmosphere
DOI: 10.1016/j.icarus.2003.11.015 Bibcode: 2004Icar..169..197J

Ballester, Gilda E.; Spencer, John R.; Howell, Robert R. +4 more

Using the Hubble Space Telescope's Space Telescope Imaging Spectrograph we have obtained for the first time spatially resolved 2000-3000 Å spectra of Io's Prometheus plume and adjoining regions on Io's anti-jovian hemisphere in the latitude range 60° N-60° S, using a 0.1″ slit centered on Prometheus and tilted roughly 45° to the spin axis. The SO …

2004 Icarus
eHST 64