Greg Stumpf
EF5
Originally posted by Glen Romine
As most folks that have hung out in cores much can tell you, the hail is located immediately north to northeast of the updraft for a layout as shown in the image above, and smaller hail often extends down the 'wing' (southern half of 'V') of the eagle shaped echo, with typically just heavy rain in the 'body' (northern half of 'V') portion of the echo. The reason for the void in between might be in part due to the perturbed flow due to the updraft, but the southward extension of the echo probably has more to do with extreme storm-top divergence fanning out the precipitation at the top of the updraft.
Glen,
You may have hit the nail on the head here. The shape of the reflectivity echo in the forward flank may be due to the distribution of hail versus rain in the core. Perhaps the reflectivity in the right "wing" of the core has more of a hail contribution, and thus appears more intense on radar.
Just a thought. It would be nice to compare storms with and without the downwind V-notch to a dense network of surface precip obs. Of course, those kinds of data sets are nearly impossible outside the realm of special field projects.