%0 Journal Article %1 w2004cassini %A Esposito, Larry W. %A Barth, Charles A. %A Colwell, Joshua E. %A Lawrence, George M. %A McClintock, William E. %A Stewart, A. Ian F. %A Keller, H. Uwe %A Korth, Axel %A Lauche, Hans %A Festou, Michel C. %A Lane, Arthur L. %A Hansen, Candice J. %A Maki, Justin N. %A West, Robert A. %A Jahn, Herbert %A Reulke, Ralf %A Warlich, Kerstin %A Shemansky, Donald E. %A Yung, Yuk L. %D 2004 %J Space Science Reviews %K cassini imaging spectrograph ultraviolet %N 1 %P 299--361 %T The Cassini Ultraviolet Imaging Spectrograph Investigation %U http://dx.doi.org/10.1007/s11214-004-1455-8 %V 115 %X The Cassini Ultraviolet Imaging Spectrograph (UVIS) is part of the remote sensing payload of the Cassini orbiter spacecraft. UVIS has two spectrographic channels that provide images and spectra covering the ranges from 56 to 118 nm and 110 to 190 nm. A third optical path with a solar blind CsI photocathode is used for high signal-to-noise-ratio stellar occultations by rings and atmospheres. A separate Hydrogen Deuterium Absorption Cell measures the relative abundance of deuterium and hydrogen from their Lyman-α emission. The UVIS science objectives include investigation of the chemistry, aerosols, clouds, and energy balance of the Titan and Saturn atmospheres; neutrals in the Saturn magnetosphere; the deuterium-to-hydrogen (D/H) ratio for Titan and Saturn; icy satellite surface properties; and the structure and evolution of Saturn’s rings. ER -

@article{w2004cassini, abstract = {The Cassini Ultraviolet Imaging Spectrograph (UVIS) is part of the remote sensing payload of the Cassini orbiter spacecraft. UVIS has two spectrographic channels that provide images and spectra covering the ranges from 56 to 118 nm and 110 to 190 nm. A third optical path with a solar blind CsI photocathode is used for high signal-to-noise-ratio stellar occultations by rings and atmospheres. A separate Hydrogen Deuterium Absorption Cell measures the relative abundance of deuterium and hydrogen from their Lyman-α emission. The UVIS science objectives include investigation of the chemistry, aerosols, clouds, and energy balance of the Titan and Saturn atmospheres; neutrals in the Saturn magnetosphere; the deuterium-to-hydrogen (D/H) ratio for Titan and Saturn; icy satellite surface properties; and the structure and evolution of Saturn’s rings. ER -}, added-at = {2010-05-16T13:31:25.000+0200}, author = {Esposito, Larry W. and Barth, Charles A. and Colwell, Joshua E. and Lawrence, George M. and McClintock, William E. and Stewart, A. Ian F. and Keller, H. Uwe and Korth, Axel and Lauche, Hans and Festou, Michel C. and Lane, Arthur L. and Hansen, Candice J. and Maki, Justin N. and West, Robert A. and Jahn, Herbert and Reulke, Ralf and Warlich, Kerstin and Shemansky, Donald E. and Yung, Yuk L.}, biburl = {https://www.bibsonomy.org/bibtex/2bb9df119fbe0ef736e2f08ca6617cbf6/gensemer}, description = {SpringerLink - Journal Article}, interhash = {ba923df1e72ee56a3b1fbdce95fca956}, intrahash = {bb9df119fbe0ef736e2f08ca6617cbf6}, journal = {Space Science Reviews}, keywords = {cassini imaging spectrograph ultraviolet}, month = {#nov#}, number = 1, pages = {299--361}, timestamp = {2010-05-16T13:31:25.000+0200}, title = {The Cassini Ultraviolet Imaging Spectrograph Investigation}, url = {http://dx.doi.org/10.1007/s11214-004-1455-8}, volume = 115, year = 2004 }