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. 6

Hemispherical albedo distribution as a function of wavelength in the range from 200 to 2500 nm for the three samples (sample A, sample B and sample C) considered in this paper. As in the case of pure analogues, an integrating sphere was used for measurements.

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