Fig. 1From: Modelling cometary meteoroid stream traverses of the Martian Moons eXploration (MMX) spacecraft en route to PhobosSimulated dust fluxes for cometary meteoroid trails intercepted by the MMX spacecraft during its interplanetary transfer to Mars (cf. Fig. 2). Simulated particles are larger than \(100\,\mu \mathrm { m}\). Symbols and colours distinguish individual comets: red crosses: 21P/Giacobini-Zinner; blue triangles: 24P/Schaumasse; blue diamonds: 45P/H-M-P; black asterisks: 103P/Hartley; green crosses: 255P/Levy; blue crosses: 207P/NEAT; green triangles: 249P/LINEAR; blue squares: 263P/Gibbs; yellow triangles: 41P/Tuttle-Giacobini-Kresák. The simulations were performed with a 1-day step size for 21P, and with a 2-day step size for all other comets. The dashed line shows the simulated flux of sporadic interplanetary dust particles, see text for detailsBack to article page