Determination of bolometric albedo based on spectroscopic measurements for selected dust analogues and its impact on the change of cometary brightness during its outburst

Open Access

Fig. 10

Distribution of changes in brightness as a function of the surface that has undergone destruction. The presented calculation results refer to model A, in which we take into account the volumetric share of dust and ice particles in their total amount contained in the coma. The calculations assumed that the parameter η₁ = 10%.

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