to store solar energy. The rise of heated (and thus less dense) water to the surface is
prevented by adding salt at the pond bottom. In a typical salt gradient solar pond, the
density of water increases in the gradient zone, as shown in Figure 3, and the density
can be expressed as
P = Po√√1+tan² (77)
where po is the density on the water surface, z is the vertical distance measured down-
ward from the top of the gradient zone, and H is the thickness of the gradient zone.
For H = 4 m, po = 1040 kg/m³, and a thickness of 0.8 m for the surface zone, calculate
the gage pressure at the bottom of the gradient zone.
Fig: 1