Figure 2From: Probing of meteor showers at Mars during the encounter of comet C/2013 A1: predictions for the arrival of MAVEN/MangalyaanMeteoroids fluxes observed by Pioneers 8 and 11, HEOS, and Pegasus satellites at 1.0 AU. These fluxes are scaled to Mars orbit at 1.5 AU. Plus (+) shows upper limit of meteoroid flux measured by Opportunity/MER rovers on Mars [7]. Solid line represents Interplanetary Dust Model of Grun et al. [19].Back to article page