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The reduction of parameter dimensions in Part I is complemented by the compaction of parameter space in Part II. The range of diameters is 0.5 ≤ D ≤ 8 cm, and the assumed liquid water content varies within 1 ≤ Wf ≤ 3 for dry growth and Wf ≤ 6 g m−3 for shedding. Entirely new data throw new light onto HMT and growth.Results are as follows: (i) dry growth is unimportant, since most hailstones grow spongy; (ii) radial growth is slow for dry and fast for spongy growth because less latent heat of freezing needs to be discarded if a smaller portion of the accreted water is frozen: this growth with shedding is particularly effective if the product Y of the net collection efficiency and ice mass fraction of the deposit is 0.2 ≤ Y ≤ 0.6; (iii) the lowest possible surface temperature tS for dry growth is −32.3°C. For water-skin-covered, spongy particles tS > −5°C, and tS > −0.55°C for shedding from wet surfaces without water skins; and (iv) the interplay between water-skin thickness and surface temperature ...

New Hailstone Physics. Part II: Interaction of the Variables