One hundred and thirty Omega dropwindsondes deployed within 500-km radius o
f the eye of six North Atlantic hurricanes are used to determine the magnit
udes and trends in convective available potential energy, and 10-1500-m and
0-6-km shear of the horizontal wind as a function of radius, quadrant, and
hurricane intensity.
The moist convective instability found at large radii (400-500 km) decrease
s to near neutral stability by 75 km from the eyewall. Vertical shears incr
ease as radius decreases, but maximum shear values are only one-half of tho
se found over land. Scatter for birth the conditional instability and the s
hear is influenced chiefly by hurricane intensity, but proximity to reflect
ivity features does modulate the pattern. The ratio of the conditional inst
ability to the shear (bulk Richardson number) indicates that supercell form
ation is favored within 250 km of the circulation center, but helicity valu
es are below the threshold to support strong waterspouts.
The difference between these oceanic observations and those made over land
by other researchers is evidence for significant modification of the vertic
al profile of the horizontal wind in a hurricane at landfall.