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Subjects

Geography

The heat budget of the earth

पृथ्वी का ऊष्मा बजट

Class 11 Geography explores the heat budget of the Earth as the balance between incoming solar radiation and outgoing terrestrial radiation. Students learn how the atmosphere, land, oceans, clouds, and ice reflect, absorb, store, and redistribute heat, and why the Earth’s average temperature remains broadly stable. The topic connects this balance with the greenhouse effect, latitudinal differences in heating, and the movement of heat through the atmosphere and oceans.

TOPIC PRACTICE

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25 questions

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Medium · Level 3
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  1. Horizontal transfer of heat
  2. Creation of solar energy
  3. Complete destruction of terrestrial radiation
  4. Permanent zeroing of albedo
Medium · Level 3
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  1. Difference between energy surplus and deficit of low and high latitudes
  2. Only difference between river and lake
  3. Only height difference between mountain and plain
  4. Only difference between day and week
Medium · Level 3
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  1. Tendency to keep rising or falling
  2. Always complete stability
  3. Destruction of the Sun
  4. Stopping of rainfall
Medium · Level 3
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  1. Clear sky low albedo and strong solar radiation
  2. Thick cloud high albedo and weak Sun
  3. Long polar night and snow surface
  4. Strong reflection and low absorption
Medium · Level 3
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  1. Clear cold night and strong terrestrial radiation
  2. Strong noon sunshine and low reflection
  3. Dark surface and high absorption
  4. Arrival of warm air
Medium · Level 3
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  1. Greater counter radiation of longwave energy
  2. Greater direct incoming solar energy
  3. Earths albedo becoming zero
  4. Heating of sound energy
Medium · Level 3
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  1. Direct escape of some longwave energy to space
  2. All solar energy stopping at surface
  3. Clouds changing into Earth
  4. Energy becoming a river
Medium · Level 3
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  1. Reflection by day and counter radiation by night
  2. Ocean formation by day and mountain formation by night
  3. Gravity by day and sound by night
  4. Dust formation by day and river formation by night
Medium · Level 3
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  1. Absorbed energy may increase
  2. Absorbed energy will always decrease
  3. Longwave emission will be impossible
  4. Solar energy will stop
Medium · Level 3
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  1. When incoming energy is greater than outgoing energy
  2. When outgoing energy is greater than incoming energy
  3. When there is no energy exchange
  4. When there is only reflection and no absorption
Medium · Level 3
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  1. When outgoing energy is greater than incoming energy
  2. When incoming energy is greater than outgoing energy
  3. When all energy is absorbed
  4. When the Sun shines more
Medium · Level 3
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  1. Because it is the other side of average temperature balance
  2. Because only outgoing energy makes rainfall
  3. Because incoming energy has no importance
  4. Because outgoing energy is always zero
Medium · Level 3
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  1. Because it explains energy distribution and temperature
  2. Because it only tells political boundaries
  3. Because it measures river length
  4. Because it only tells soil texture
Medium · Level 3
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  1. Solar energy arrives some is reflected some is absorbed and Earth sends out longwave energy
  2. Solar energy arrives and never leaves
  3. All energy stays only in clouds
  4. Earth receives energy only from the Moon
Medium · Level 3
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  1. It helps keep climate stable in the long term
  2. It stops Earth's rotation
  3. It removes ocean salinity
  4. It makes mountain heights equal
Medium · Level 3
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  1. The Sun has a much higher temperature than Earth
  2. Earth is hotter than the Sun
  3. The Moon changes the radiation
  4. Oceans block all waves
Medium · Level 3
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  1. Available heat decreases
  2. Available heat always doubles
  3. Solar radiation stops forming
  4. Terrestrial radiation ends
Medium · Level 3
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  1. They reflect solar energy by day and trap longwave heat at night
  2. They create the Sun in both day and night
  3. They change Earth's revolution
  4. They instantly freeze oceans
Medium · Level 3
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  1. Longwave terrestrial radiation
  2. Shortwave solar radiation
  3. Sound wave
  4. Tidal energy
Medium · Level 3
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  1. Absorption of solar energy will increase
  2. Reflection will greatly increase
  3. Heat budget will end
  4. The Sun will stop sending radiation
Medium · Level 3
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  1. Sun rays are oblique and energy spreads out
  2. Earth does not rotate there
  3. There is no atmosphere there
  4. The Sun is always closer there
Medium · Level 3
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  1. Sun rays fall more directly
  2. Clouds never form there
  3. Earth gives energy to the Sun there
  4. Longwave radiation does not occur there
Medium · Level 3
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  1. It absorbs reflects and scatters radiation
  2. It stops the Sun from giving energy
  3. It makes Earth flat
  4. It separates oceans from energy
Medium · Level 3
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  1. It helps maintain the temperature of the lower atmosphere
  2. Earth's gravity ends
  3. The Sun's temperature decreases
  4. Oceans dry instantly
Medium · Level 3
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  1. Total received energy and total emitted energy remain nearly equal
  2. Earth never emits energy
  3. All energy goes only into oceans
  4. Atmosphere destroys energy

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