a) - The
solar constant is a flux density measuring
mean solar electromagnetic radiation (
solarirradiance) per unit area. It is measured on a surface perpendicular to the rays, one astronomical unit (AU) from the
Sun (roughly the distance from the
Sun to the Earth).
The approximate average value cited,
1.3608 ± 0.0005 kW/m², which is 81.65 kJ/m² per minute, is equivalent to
approximately 1.951calories per minute per square centimeter, or
1.951 langleys per minute. Solar output is nearly, but not quite, constant.
b) -
i
E = 4200 kJ
t = 10 min = 600 sec
P = E/t = 7 kJ/sec
Area = 5 m²
P/A = 7/5 = 1.4 kJ/sec m²
This is the value of the solar constant.
This means that 1.4 kJ of solar energy reaches the surface of the earth in 1 second over an area of 1m².