Generation of inertia-gravity waves by a time-dependent baroclinic wave in the laboratory
PHYSICS AND CHEMISTRY OF THE EARTH PART B-HYDROLOGY OCEANS AND ATMOSPHERE 24:5 (1999) 455-460
Improved general circulation models of the Martian atmosphere from the surface to above 80 km
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 104:E10 (1999) 24155-24175
The effect of sloping boundaries on baroclinic instability in two related internally heated, rotating fluid systems
PHYSICS AND CHEMISTRY OF THE EARTH PART B-HYDROLOGY OCEANS AND ATMOSPHERE 24:5 (1999) 481-486
Investigation of Saturn's atmosphere by Cassini
PLANET SPACE SCI 46:9-10 (1998) 1315-1324
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.A comparison of empirical orthogonal decomposition methods in baroclinic flows
Dynamics of Atmospheres and Oceans 27:1-4 (1998) 649-660