Figures & data
FIG. 1 Normalized cumulative weight distributions of penetrating particles predicted by the Calvert theoretical model and optimally fitted by lognormal distributions.
![FIG. 1 Normalized cumulative weight distributions of penetrating particles predicted by the Calvert theoretical model and optimally fitted by lognormal distributions.](/cms/asset/2850aeec-0b33-489b-aa33-bf1dc5ea239f/uast_a_211220_o_f0001g.gif)
FIG. 2 (a) Nomographs based on the Calvert formulation, for Bf = 1.4, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (b) Nomographs based on the Calvert formulation, for Bf = 1.6, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (c) Nomographs based on the Calvert formulation, for Bf = 1.9, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (d) Nomographs based on the Calvert formulation, for Bf = 2.3, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (e) Nomographs based on the Calvert formulation, for Bf = 3, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (f) Nomographs based on the Calvert formulation, for Bf = 4, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (g) Nomographs based on the Calvert formulation, for Bf = 6, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (h) Nomographs based on the Calvert formulation, for Bf = 16, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g .
![FIG. 2 (a) Nomographs based on the Calvert formulation, for Bf = 1.4, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (b) Nomographs based on the Calvert formulation, for Bf = 1.6, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (c) Nomographs based on the Calvert formulation, for Bf = 1.9, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (d) Nomographs based on the Calvert formulation, for Bf = 2.3, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (e) Nomographs based on the Calvert formulation, for Bf = 3, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (f) Nomographs based on the Calvert formulation, for Bf = 4, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (g) Nomographs based on the Calvert formulation, for Bf = 6, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g . (h) Nomographs based on the Calvert formulation, for Bf = 16, yielding the output particle distribution parameters G c d pα and lnσ p as function of the input particle distribution parameters G c d mα and lnσ g .](/cms/asset/b15eacbe-aa2d-4618-b100-dc96de82b9d8/uast_a_211220_o_f0002g.gif)
FIG. 3 Algorithm for generating best-fit lognormal distribution parameters d p and σ p from cumulative weight fraction series computed through the use of Calvert and Yung et al. formulations.
![FIG. 3 Algorithm for generating best-fit lognormal distribution parameters d p and σ p from cumulative weight fraction series computed through the use of Calvert and Yung et al. formulations.](/cms/asset/a725148a-18e5-4ae5-9df7-6be878c5553a/uast_a_211220_o_f0003g.gif)