Fig. 2
Dimensionless efficiency factor for the radiation pressure (
) determined for totally reflecting particles (solid line). Spectral distribution of Planck’s blackbody with temperature 5500 K in dependence on xM = 2πR/λ for R = 0.168 μm is shown for comparison (dashed line). The maximal 
is obtained for the dust particle with R = 0.168 μm.
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