Solar Radiation, Heat Balance and Temperature
Madhya Pradesh Board · Class 11 · Geography
Summary of Solar Radiation, Heat Balance and Temperature for Madhya Pradesh Board Class 11 Geography. Key concepts, important points, and chapter overview.
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Overview
Solar energy reaches Earth mainly as short-wave radiation called insolation. The atmosphere is mostly transparent to this radiation, but some of it is absorbed, scattered, and reflected. Earth then returns energy to space as long-wave terrestrial radiation. This continuous exchange keeps the planet
Key Concepts
Incoming solar radiation received by
Incoming solar radiation received by the Earth is called insolation. The Earth receives it mainly in short wavelengths, and on average it gets 1.94 ca
Earth is farthest from the Sun
Earth is farthest from the Sun on 4th July at 152 million km, called aphelion. Earth is nearest to the Sun on 3rd January at 147 million km, called pe
The amount of insolation varies because
The amount of insolation varies because of Earth’s rotation, the angle of inclination of the Sun’s rays, length of day, transparency of the atmosphere
The atmosphere is largely transparent
The atmosphere is largely transparent to short-wave solar radiation. Water vapour, ozone, and other gases absorb much of the near-infrared radiation w
Insolation at the surface ranges from
Insolation at the surface ranges from about 320 Watt/m² in the tropics to about 70 Watt/m² at the poles. Maximum insolation occurs over subtropical de
Learning Objectives
- Understand the meaning of insolation and how it reaches Earth
- Explain why solar radiation varies with latitude, season, and time of day
- Describe conduction, convection, and advection as methods of heat transfer
- Explain terrestrial radiation and the heat budget of the Earth
- Understand the meaning of temperature and factors controlling its distribution
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