Turbulent fluxes have been evaluated for clear sunny days over the Ind
ian Antarctic station, Maitri, using the basic meteorological data rec
orded at four levels of a 28 m tower. The data are supplemented with r
adiation data. The surface layer over Maitri remains thermally stratif
ied during the hours of minimum solar insolation, the so-called nightt
ime period. The surface winds during this period are generally very st
rong resulting in high momentum fluxes. In particular, for high winds
(>12 m s(-1)), the temperature gradient is found to be less positive t
han for moderate winds (4 to 7 m s(-1)). Solar insolation provided the
daytime heating necessary for the diurnal variation of atmospheric st
ability, and hence, for the turbulent fluxes. Thus, on clear days dayt
ime conditions are marked by upward transport of heat with reduced mom
entum flux, while stable nighttime conditions are marked by a downward
heat flux with increased momentum fluxes.