In Rayleigh Bénard convection, for a range of Prandtl numbers
$4.69 \leqslant Pr \leqslant 5.88$
and Rayleigh numbers
$5.52\times 10^5 \leqslant Ra \leqslant 1.21\times 10^9$
, we study the effect of shear by the inherent large-scale flow (LSF) on the local boundary layers on the hot plate. The velocity distribution in a horizontal plane within the boundary layers at each
$Ra$
, at any instant, is (A) unimodal with a peak at approximately the natural convection boundary layer velocities
$V_{bl}$
; (B) bimodal with the first peak between
$V_{bl}$
and
$V_{L}$
, the shear velocities created by the LSF close to the plate; or (C) unimodal with the peak at approximately
$V_{L}$
. Type A distributions occur more at lower
$Ra$
, while type C occur more at higher
$Ra$
, with type B occurring more at intermediate
$Ra$
. We show that the second peak of the bimodal type B distributions, and the peak of the unimodal type C distributions, scale as
$V_{L}$
scales with
$Ra$
. We then show that the areas of such regions that have velocities of the order of
$V_{L}$
increase exponentially with increase in
$Ra$
and then saturate. The velocities in the remaining regions, which contribute to the first peak of the bimodal type B distributions and the single peak of type A distributions, are also affected by the shear. We show that the Reynolds number based on these velocities scale as
$Re_{bs}$
, the Reynolds number based on the boundary layer velocities forced externally by the shear due to the LSF, which we obtained as a perturbation solution of the scaling relations derived from integral boundary layer equations. For
$Pr=1$
and aspect ratio
$\varGamma =1$
,
$Re_{bs} \sim Ra^{0.375}$
for small shear, similar to the observed flux scaling in a possible ultimate regime. The velocity at the edge of the natural convection boundary layers was found to increase with
$Ra$
as
$Ra^{0.35}$
; since
$V_{bl}\sim Ra^{1/3}$
, this suggests a possible shear domination of the boundary layers at high
$Ra$
. The effect of shear, however, decreases with increase in
$Pr$
and with increase in
$\varGamma$
, and becomes negligible for
$Pr\geqslant 100$
at
$\varGamma =1$
or for
$\varGamma \geqslant 20$
at
$Pr=1$
, causing
$Re_{bs}\sim Ra_w^{1/3}$
.