Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method

<table class="table-group" id="tab3"><tr><td><table class="table"><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr class="thead"><td class="align_left">Simulation parameters</td><td class="align_center">Value</td></tr><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr><td class="align_left">Operating pressure</td><td class="align_center">690 pa</td></tr><tr><td class="align_left">Gravity</td><td class="align_center">3.73 m/s<sup>2</sup></td></tr><tr><td class="align_left">Temperature</td><td class="align_center">220 K</td></tr><tr><td class="align_left">Density</td><td class="align_center">0.0167 kg/m<sup>3</sup></td></tr><tr><td class="align_left">Viscosity</td><td class="align_center"><span style="width: 111.85ptpx;"><svg height="14.9947pt" id="M142" style="vertical-align:-3.4033pt" version="1.1" viewbox="-0.0498162 -11.5914 111.85 14.9947" width="111.85pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g 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<div>CFD simulation parameters of Martian airflow in Fluent.</div>

International Journal of Aerospace Engineering

tab3

Table 3

Table 3: Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method 