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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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