A
Arthur L. Lane
Researcher at California Institute of Technology
Publications - 133
Citations - 4336
Arthur L. Lane is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Rings of Saturn & Spectrometer. The author has an hindex of 38, co-authored 132 publications receiving 4116 citations. Previous affiliations of Arthur L. Lane include Jet Propulsion Laboratory.
Papers
More filters
Journal ArticleDOI
The Cassini Ultraviolet Imaging Spectrograph Investigation
Larry W. Esposito,Charles A. Barth,Joshua Colwell,George M. Lawrence,William E. McClintock,A. Ian F. Stewart,H. Uwe Keller,A. Korth,Hans Lauche,Michel C. Festou,Arthur L. Lane,Candice Hansen,Justin N. Maki,Robert A. West,Herbert Jahn,Ralf Reulke,Kerstin Warlich,Donald E. Shemansky,Yuk L. Yung +18 more
TL;DR: The Cassini Ultraviolet Imaging Spectrograph (UVIS) as discussed by the authors is part of the remote sensing payload of the Cassini orbiter spacecraft and has two spectrographic channels that provide images and spectra covering the ranges from 56 to 118 nm and 110 to 190 nm.
Journal ArticleDOI
Photopolarimetry from Voyager 2; Preliminary Results on Saturn, Titan, and the Rings
Arthur L. Lane,Charles W. Hord,Robert A. West,Larry W. Esposito,D. L. Coffeen,Makiko Sato,Karen E. Simmons,Richard B. Pomphrey,Richard B. Morris +8 more
TL;DR: The Voyager 2 photopolarimeter was reprogrammed prior to the August 1981 Saturn encounter to perform orthogonal-polarization, two-color measurements on Saturn, Titan, and the rings, and multiple, very narrow strands of material were found in the Encke division and within the brightest single strand of the F ring.
Journal ArticleDOI
Evidence for sulphur implantation in Europa's UV absorption band
TL;DR: In this paper, the spectral characteristics of the Galilean satellites were investigated using data from the International Ultraviolet Explorer (IUE) spacecraft as a function of the orbital position, large-scale areal variability, and temporal dynamics.
Journal ArticleDOI
Detection of Ozone on Ganymede
TL;DR: An absorption band at 260 nanometers on the trailing hemisphere of Ganymede, identified as the Hartley band of ozone (O3), was measured with the Hubble Space Telescope, and apparently this O2-O3 “atmosphere” is trapped in GanyMede's surface ice, an inference consistent with the shift and broadening of the band.
Journal ArticleDOI
Mariner 9 Ultraviolet Spectrometer Experiment: Seasonal Variation of Ozone on Mars
Charles A. Barth,Charles W. Hord,A. Ian F. Stewart,Arthur L. Lane,Mary L. Dick,Gail P. Anderson +5 more
TL;DR: Ozone is observed to be present in the polar regions of Mars and to have a seasonal variation, and is found in association with the formation of the polar hood.