Fig. 4.29 Numerical solutions to the dust distribution for an insolation-driven spherical nucleus of
2 km in diameter for three different particle sizes. The rows indicate (top to bottom) the local dust
density, the dust speed, the radial component of the dust speed, and the drag coefficient (from
Marschall 2017)
332
4 Dust Emission from the Surface
2 km in diameter for three different particle sizes. The rows indicate (top to bottom) the local dust
density, the dust speed, the radial component of the dust speed, and the drag coefficient (from
Marschall 2017)
332
4 Dust Emission from the Surface