Predicting weather conditions and climate for Mars expeditions
SCI TECH 107 (2004) 3-21
Abstract:
Weather and climatic conditions are among the most important factors to be taken into account when planning expeditions to remote and challenging locations on Earth. This is likely to be equally the case for expedition planners on Mars, where conditions (in terms of extremes of temperature, etc.) can be at least as daunting as back on Earth. With the success of recent unmanned missions to Mars, such as NASA's Mars Pathfinder, Mars Global Surveyor and Mars Odyssey, there is now a great deal of information available on the range of environmental conditions on Mars, from the tropics to the CO2 ice-covered polar caps. This has been further supplemented by the development of advanced numerical models of the Martian atmosphere, allowing detailed and accurate simulations and predictions of the weather and climate across the planet. This report discusses the main weather and climate variables which future Martian human expedition planners will need to take into account. The range of conditions likely to be encountered at a variety of typical locations on Mars is then considered, with reference to predictions from the ESA Mars Climate Database.Stochastic resonance in a nonlinear model of a rotating, stratified shear flow, with a simple stochastic inertia-gravity wave parameterization
NONLINEAR PROCESSES IN GEOPHYSICS 11:1 (2004) 127-135
The Martian climate revisited
Springer Verlag, 2004
Abstract:
latest techniques of atmospheric modelling, The Martian Climate Revisited provides a comprehensive summary of our knowledge and current understanding of the meteorology and climate of Mars from the viewpoint of atmospheric scientists .The effect of a global dust storm on simulations of the Martian water cycle -: art. no. L22702
GEOPHYSICAL RESEARCH LETTERS 31:22 (2004) ARTN L22702
Upper atmosphere of Mars up to 120 km:: Mars Global Surveyor accelerometer data analysis with the LMD general circulation model -: art. no. E01011
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 109:E1 (2004) ARTN E01011