By A. J. Chisholm, Marianne English (auth.)
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In Case 3 of Fig. 54, the relative winds appear to have resulted in an extreme tilt to the upper branch of the storm updraft. With a stronger updraft, this effect would not likely have been so pronounced. Ultimately, the relative winds above cloud base must influence the direction of storm outflow and the region of precipitation fallout. This effect is particularly pronounced in Case 3. N RADAR 29 JUNE 1967 ~ STORM MOTION ~ From the above-mentioned points there appear to be three controlling influences which determine the structure and character of a severe storm.
Ind components relative to the storm (in the plane of storm motion) are shown on the left-hand side. The inflow air is shown to enter the storm on the upwind side, ascending upward through the UWER, while tilting downwind. The outflow air exits downstream under the influence of the moderately strong wind component relative to the storm, and the precipitation particles would be expected to fall through the Z, maximum downwind from the updraft. 1356 (see Chisholm, 1970a), each displays essentially the same features exhibited by Figs.
Newton, C. , 1963: Dynamics of severe convective storms. Meteor. , 5, No. 27, 33-58. - - , 1966: Circulations in large sheared cumulonimbus. Tellus, 18, 699-713. Probert-Jones, J. , 1962: The radar equation in meteorology. Quart. J. Roy. Meteor. , 88, 485--495. Stackpole, J. , 1967: Numerical analysis of atmospheric soundings. J. Appl. , 6, 461--466. ALBERTA HAILSTORMS PART II: GROWTH OF LARGE HAIL IN THE STORM MARIANNE ENGLISH 1 ~McGill University, Montreal, Canada ABSTRACT The growth of hail in four different storms has been modeled successfully by a single procedure.