• Solar pyrolysis process of willow pellet is dynamically studied. • The effect of thickness and heat flux density on product yields is analyzed. • The intra-particle secondary reactions of volatile composition are further studied. • Dimensionless number Bi∙Prmass is proposed to predict solar pyrolysis behavior. • Mechanism of volatile evolution during solar pyrolysis is revealed. To study the volatile evolution mechanism during solar pyrolysis of biomass, willow pellets with thicknesses of 3 mm, 1 mm and 0.5 mm were used to investigate the dynamic pyrolysis characteristics at heat flux densities of 0.5 and 1.1 MW/m 2 . The results showed that the larger thickness significantly reduced oil yield (by 23%–35%) and increases gas yield (by 19%–20%), while increasing heat flux density showed a similar trend. These changes in solar pyrolysis behavior and product composition were governed by intra-particle secondary reactions due to the heat and mass transfer conditions. The evolution of heavy compounds (molecular weight ≥ 200 Da) was integrated into the volatile evolution mechanism of solar pyrolysis. Results showed the secondary reactions promoted the cracking, deoxygenation and condensation of sugars and phenolic species, and also led to the growth of condensed aromatic hydrocarbons. A novel dimensionless number (Bi∙Pr mass ) was proposed in this study to estimate the solar pyrolysis behavior of wood pellets. A smaller Bi∙Pr mass indicates that the conversion process is dominated by primary pyrolysis, while a higher value indicates that it is dominated by intra-particle secondary reactions. Depending on the degree of condensation, a critical value of Bi∙Pr mass around 0.1 was adopted in this study. This work can provide guidance about operating conditions optimization for solar gasification of biomass.
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