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Evidence for control of Atlantic subtropical humidity by large scale advection

Geophysical Research Letters American Geophysical Union (AGU) 25:24 (1998) 4537-4540

Authors:

Raymond T Pierrehumbert, Rémy Roca
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Virtis : an imaging spectrometer for the rosetta mission

Planetary and Space Science Elsevier 46:9-10 (1998) 1291-1304

Authors:

A Coradine, F Capaccioni, P Drossart, A Semery, G Arnold, U Schade, F Angrilli, MA Barucci, G Bellucci, G Bianchini, JP Bibring, A Blanco, M Blecka, D Bockelee-Morvan, R Bonsignori, M Bouye, E Bussoletti, MT Capria, R Carlson, U Carsenty, P Cerroni, L Colangeli, M Combes, M Combi, J Crovisier, M Dami, MC DeSanctis, AM DiLellis, E Dotto, T Encrenaz, E Epifani, S Erard, S Espinasse, A Fave, C Federico, U Fink, S Fonti, V Formisano, Y Hello, H Hirsch, G Huntzinger, R Knoll, D Kouach, WH Ip, P Irwin, J Kachlicki, Y Langevin, G Magni, T McCord, V Mennella, H Michaelis, G Mondello, S Mottola, G Neukum, V Orofino, R Orosei, P Palumbo, G Peter, B Pforte, G Piccioni, JM Reess, E Ress, B Saggin, B Schmitt, Stefanovitch, A Stern, F Taylor, D Tiphene, G Tozzi
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Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia

Journal of Geophysical Research American Geophysical Union (AGU) 103:E10 (1998) 23023-23041

Authors:

M Roos‐Serote, P Drossart, T Encrenaz, E Lellouch, RW Carlson, KH Baines, L Kamp, R Mehlman, GS Orton, S Calcutt, P Irwin, F Taylor, A Weir
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The solar reflected component in Jupiter's 5‐μm spectra from NIMS/Galileo observations

Journal of Geophysical Research American Geophysical Union (AGU) 103:E10 (1998) 23043-23049

Authors:

P Drossart, M Roos‐Serote, T Encrenaz, E Lellouch, KH Baines, RW Carlson, LW Kamp, GS Orton, S Calcutt, P Irwin, FW Taylor, A Weir
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Investigation of Saturn's atmosphere by Cassini

PLANET SPACE SCI 46:9-10 (1998) 1315-1324

Authors:

FW Taylor, SB Calcutt, PGJ Irwin, CA Nixon, PL Read, PJC Smith, TJ Vellacott

Abstract:

This paper considers the rationale for the exploration of Saturn's atmosphere by the Cassini mission, taking account of the key scientific questions posed by the earlier investigation by Voyager, and the capabilities of the instrumentation making up the Cassini payload. While by no means all objectives can be addressed by this particular configuration, in particular without a Saturn entry probe, if everything goes according to plan important progress should be possible on a number of key objectives. (C) 1998 Elsevier Science Ltd. All rights reserved.
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