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Class 11 Solar Radiation, Heat Balance and Temperature: cheat sheet

CBSE Social Science. How the earth is heated by the sun, how the atmosphere is heated and cooled, the heat budget, the lapse rate and the spread of temperature.

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Key ideas

Remember

Normal lapse rate6.5 °C fall per 1,000 m (1.3 °C per 200 m)
Temperature at a heightsurface temperature − height in m × 6.5 ÷ 1,000
Height from a temperature gapdifference in °C ÷ 6.5 × 1,000 m
Annual rangewarmest month − coldest month (careful with minus signs)
Heat budget (of 100 units)35 reflected; 65 absorbed (14 by the air, 51 by the surface); 17 + 48 = 65 radiated to space
Perihelion and aphelionnearest to the sun on 3rd January (147 million km), farthest on 4th July (152 million km)
Most insolationover the subtropical deserts (least cloud), not at the equator

Watch out

Worked example

A climber starts at sea level, where it is 30 °C, and reaches 6,400 m. Using 6.5 °C per 1,000 m: (a) What is the temperature at 2,000 m? (b) At the top? (c) Why does temperature fall with height?

Working: 30 − 2,000 × 6.5 ÷ 1,000; 30 − 6,400 × 6.5 ÷ 1,000

Answer: (a) 17 °C (b) −11.6 °C (c) The air is heated from below by terrestrial radiation and is thinner higher up.

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