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The science
Plume height. Mastin et al. (2009) fitted observed eruptions: H = 2.00 V^0.241 with H in km above the vent and V the dense-rock-equivalent volume rate in m3/s; mass rate = 2500 kg/m3 x V. VEI is estimated from the erupted mass over one hour, log10(M/kg) - 7.
Terminal velocity. A grain stops accelerating when drag equals buoyant weight: (1/2) Cd rho_a v^2 (pi d^2/4) = (rho_p - rho_a) g (pi d^3/6) with the drag coefficient Cd(Re) of a sphere. For small grains (Re < 1) this reduces to Stokes: v = (rho_p - rho_a) g d^2 / (18 mu). The sim solves the full balance by bisection and shows both curves.
Fallout. Each grain is advected by the wind u(z) and falls at v: with uniform wind the landing distance is x = u z0 / v (checked in-page against the stepper). A turbulent diffusivity K spreads grains randomly. The deposit graph is mass landed per kilometre downwind.
Simplifications. Constant air density and viscosity, spherical grains of 2300 kg/m3, one wind direction with linear shear, a schematic bent-over column, number-weighted grain sizes, no aggregation of fine ash, no pyroclastic flows. Treat distances as order-of-magnitude estimates.