摘要 : <![CDATA[<ce:abstract xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns="http://www.elsevier.com/xml/ja/dtd" class="author-highlights" id="absh001" view="all"> <ce:section-title id="sectt0001">Highlights</ce:section-title> <... 展开 <![CDATA[<ce:abstract xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns="http://www.elsevier.com/xml/ja/dtd" class="author-highlights" id="absh001" view="all"> <ce:section-title id="sectt0001">Highlights</ce:section-title> <ce:abstract-sec id="abssec0001" view="all"> <ce:simple-para id="spara0001" view="all"> <ce:list id="celist0001"> <ce:list-item id="celistitem0001"> <ce:label>?</ce:label> <ce:para id="para0001" view="all">We perform mesoscale simulations of the water cycle in a region around Gale crater.</ce:para> </ce:list-item> <ce:list-item id="celistitem0002"> <ce:label>?</ce:label> <ce:para id="para0002" view="all">Regolith interaction reduces vapour abundances at crater floor by factors of 2-3.</ce:para> </ce:list-item> <ce:list-item id="celistitem0003"> <ce:label>?</ce:label> <ce:para id="para0003" view="all">Nighttime subsurface ice amounts are small in all seasons.</ce:para> </ce:list-item> <ce:list-item id="celistitem0004"> <ce:label>?</ce:label> <ce:para id="para0004" view="all">Diffused vapour is transported up into the atmosphere at convergence boundaries.</ce:para> </ce:list-item> <ce:list-item id="celistitem0005"> <ce:label>?</ce:label> <ce:para id="para0005" view="all">Results at Gale crater are representative of other craters in the mesoscale domain.</ce:para> </ce:list-item> </ce:list> </ce:simple-para> </ce:abstract-sec> </ce:abstract><ce:abstract xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns="http://www.elsevier.com/xml/ja/dtd" id="abs0001" class="author" view="all"> <ce:section- 收起