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PDF version of COSPAR - Space Science Research in Canada Report

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oundary layer on Mars is generally higher than on Earth—perhaps four to fivekilometres dur<strong>in</strong>g the day <strong>in</strong> the Arctic because <strong>of</strong> solar heat<strong>in</strong>g, and less at night.“We th<strong>in</strong>k the lidar will be able to tell us is how deep the boundary layer is,” hesaid. “We’re hop<strong>in</strong>g it will detect a horizon—a change <strong>in</strong> the dust concentration atlevels correspond<strong>in</strong>g to the top <strong>of</strong> the boundary layer.” This will depend on thesize <strong>of</strong> the dust particles. If they are large enough to settle out <strong>of</strong> the atmospheresufficiently rapidly at night, scientists will see the top <strong>of</strong> the boundary layer.Unfortunately, some Martian dust is very f<strong>in</strong>e and, once stirred up, settles veryslowly, if at all.The MET science team is <strong>in</strong>terpret<strong>in</strong>g the data collected on the planet by us<strong>in</strong>gcomputer models similar to those used for weather forecast<strong>in</strong>g and climateprediction on Earth to analyze the atmospheric chemistry <strong>of</strong> Mars and the roleplayed by dust.Prepar<strong>in</strong>g for the missionLong before land<strong>in</strong>g, while MDA was build<strong>in</strong>g the <strong>in</strong>struments, the Canadianscientific team conducted studies and tests to prepare for the research programdur<strong>in</strong>g spacecraft operations. The York team, for example, tested components <strong>of</strong>the temperature sensor taken from the same manufactur<strong>in</strong>g batch as thosedest<strong>in</strong>ed for the spacecraft and also built and tested a lidar technically similar tothat dest<strong>in</strong>ed for Mars.Taylor and his students participated <strong>in</strong> an <strong>in</strong>vestigation that prompted a designchange <strong>in</strong> the <strong>in</strong>strument used to collect sub-surface ice samples. From hisprevious research on blow<strong>in</strong>g snow, Taylor knew that when snow is blownaround, it sublimates—changes from a solid to a vapour. He began to wonder ifthis would happen to the ice dug up with a fork-like device on the end <strong>of</strong> therobotic arm on Phoenix—a laborious process that would take several hours.“It seemed to us that scrap<strong>in</strong>g these little chips <strong>of</strong> ice up and deliver<strong>in</strong>g them tothe analysis <strong>in</strong>strument several hours later could be a problem. We thought theseice chips would sublimate. If it takes them several hours to collect a large enoughsample, they’ll never be able to do it because the sample will vaporize.” His <strong>in</strong>itialcalculations suggested that, at a temperature <strong>of</strong> –30 degrees Celsius, the chipswould last only half an hour.This theory was greeted with some skepticism so Taylor had a student who waswork<strong>in</strong>g <strong>in</strong> the Canadian Arctic do some experiments up there. He and someother students also conducted experiments <strong>in</strong> a chamber at York that simulatesMartian conditions. “We found that if the temperature stays below about –4053

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