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Cassini infrared Fourier spectroscopic investigation

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 2803 (1996) 162-177

Authors:

Virgil G Kunde, Peter AR Ade, Richard D Barney, D Bergman, Jean-Francois Bonnal, R Borelli, David Boyd, John C Brasunas, Gregory V Brown, Simon B Calcutt, F Carroll, R Courtin, Jacky B Cretolle, Julie A Crooke, Martin A Davis, S Edberg, Rainer K Fettig, M Flasar, David A Glenar, S Graham, John G Hagopian, Claef F Hakun, Patricia A Hayes, L Herath, Linda Spilker, Donald E Jennings, Gabriel Karpati, C Kellebenz, Brook Lakew, J Lindsay, J Lohr, James J Lyons, Robert J Martineau, Anthony J Martino, Mack Matsumura, J McCloskey, T Melak, Guy Michel, Armando Morrell, C Mosier, LaTunia G Pack, M Plants, D Robinson, Louis Rodriguez, Paul Romani, Bill Schaefer, Stephen M Schmidt, Carlos Trujillo, Tim Vellacott, K Wagner, D Yun
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A second intercomparison of 222Rn measurement systems in European laboratories

Applied Radiation and Isotopes Elsevier 47:9-10 (1996) 835-840

Authors:

JCJ Dean, SA Woods, NE Bowles
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Anomalous scaling of high cloud variability in the tropical Pacific

Geophysical Research Letters American Geophysical Union (AGU) 23:10 (1996) 1095-1098
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Standardisation and measurement of the decay scheme data of 243Am and 239Np

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 369:2-3 (1996) 472-476

Authors:

SA Woods, DH Woods, MJ Woods, SM Jerome, M Burke, NE Bowles, SEM Lucas, C Paton Walsh
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Calculated k distribution coefficients for hydrogen- And self-broadened methane in the range 2000-9500 cm-1 from exponential sum fitting to band-modelled spectra

Journal of Geophysical Research: Planets 101:E11 (1996) 26137-26154

Authors:

PGJ Irwin, SB Calcutt, FW Taylor, AL Weir

Abstract:

The spectral band data derived by Strong et al. [1993] for laboratory-measured transmission spectra of hydrogen-broadened methane at 10 cm-1 resolution have been fitted with k coefficients over a wide range of pressures and temperatures representing those likely to be encountered in the atmosphere of Jupiter. The mean fitting error is found to be only 2.0×10-3 in transmission. These data are essential for the scattering calculations likely to be necessary for analysis of the data from the Near Infrared Mapping Spectrometer aboard the NASA Galileo spacecraft. The new data have significant advantages over those previously derived by Baines et al. [1993] in that they cover a wider spectral range, are applicable to longer paths, and also apply to the hydrogen-broadened case, which is the dominant broadening mechanism in this atmosphere. A similar table has also been calculated for the self-broadening case for comparison. Copyright 1996 by the American Geophysical Union.
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