Not all of the solar radiation incident on the Earth's upper atmosphere reaches the Earth's surface. The proportion R of solar radiation incident on the Earth's surface is given by: R=\frac{\text { solar power per } \mathrm{m}^{2} \text { incident on the Earth's surface }}{\text { solar power per } \mathrm{m}^{2} \text { incident on the Earth's upper atmosphere }} Solar radiation is incident normally on the surface of the solar panel with a power of 2.2 x 10³ W. Calculate R. total power output of Sun = 3.85 x 1026 W distance between Earth and Sun = 1.50 × 10¹¹ mof th area of the upper surface of the panel = 5.5 m² The rate of flow of water through the panel is 45 g s¹.TH of water through the panel is 45 g s '.The water enters the panel at a temperature of 15 °C and absorbs energy from the panel at a rate of 1.7 kW.bon Calculate the temperature of the water as it leaves the panel. \text { specific heat capacity of water }=4200 \mathrm{~J} \mathrm{~kg}^{-1} \mathrm{~K}^{-1}
Fig: 1
Fig: 2
Fig: 3
Fig: 4
Fig: 5
Fig: 6
Fig: 7
Fig: 8
Fig: 9
Fig: 10
Fig: 11
Fig: 12
Fig: 13
Fig: 14