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Geography

The heat budget of the earth

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.

Medium · Level 9 · 25 questions

TOPIC PRACTICE

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25 questions

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  1. Initial ice loss can expose darker surfaces, increase solar-energy absorption, and cause further melting
  2. Ice always produces energy
  3. Albedo is unrelated to temperature
  4. Melting ice stops incoming solar energy
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  1. When trapping of outgoing longwave radiation is stronger than reflection of incoming shortwave radiation
  2. When clouds reflect all incoming solar energy
  3. When clouds remove the atmosphere
  4. When clouds reduce the solar constant to zero
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  1. Winds and ocean currents transport heat from lower latitudes
  2. Insolation is always high at the poles
  3. Longwave radiation does not occur there
  4. The poles are sources of the Sun
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  1. The deficit will decrease
  2. The deficit may become more pronounced
  3. Solar energy will start forming
  4. Albedo will become zero
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  1. Energy spreads over a larger area, and the rays travel through a longer atmospheric path
  2. Energy travels directly to Earth's core
  3. The Sun begins emitting longwave radiation
  4. The surface produces solar energy
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  1. Because a larger share of the available energy can be used for evaporation as latent heat
  2. Because moisture destroys solar energy
  3. Because moisture prevents the surface from emitting radiation
  4. Because conduction stops completely
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  1. When evaporation takes energy from the surface and condensation releases that energy into the atmosphere
  2. When rocks become hard
  3. When a river deposits sediment
  4. When the solar constant remains unchanged
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  1. Some aerosols scatter or reflect incoming sunlight, while others absorb radiation
  2. All aerosols produce sunlight
  3. Aerosols turn longwave radiation into soil
  4. Aerosols stop Earth from orbiting the Sun
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  1. Comparing an irrigated field with dry paved ground under the same insolation
  2. Measuring the distance between the Sun and the Moon
  3. Finding an earthquake's epicentre
  4. Memorising names related to ocean salinity
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  1. Local cloud cover, surface moisture, winds, and seasonal sunlight vary.
  2. Global heat balance is an incorrect concept.
  3. Earth emits no radiation.
  4. All places have identical conditions.
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  1. It absorbs more solar energy, but its temperature may rise slowly.
  2. It reflects all incoming energy.
  3. Its temperature immediately falls to zero.
  4. Solar radiation cannot reach it.
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  1. Because absorbed solar energy and downward atmospheric radiation may also be sufficiently high.
  2. Because radiation is unrelated to temperature.
  3. Because the surface loses no energy.
  4. Because the Sun emits longwave radiation.
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  1. A large increase in albedo that reduces absorbed shortwave radiation.
  2. A large increase in the atmosphere’s absorption of outgoing longwave radiation.
  3. Clouds trapping more outgoing longwave radiation at night.
  4. The oceans storing more heat from the surface.
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  1. Cooling tendency
  2. Warming tendency
  3. No change in energy balance under all conditions
  4. Reflection-only tendency
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  1. Because both the surface and atmosphere absorb and emit energy, and the atmosphere also reradiates energy
  2. Because the surface does not absorb or emit energy
  3. Because solar radiation is absorbed only by the atmosphere
  4. Because oceans do not absorb radiation
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  1. High albedo and high evaporation
  2. Low albedo and low evaporation
  3. Very strong downward longwave radiation and little evaporation
  4. Very low heat capacity and no reflection
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  1. It is a negative feedback that tends to restore the energy balance
  2. It is a positive feedback that increases albedo
  3. It creates the solar constant
  4. It stops Earth’s rotation
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  1. Warmer air can contain more water vapour, which absorbs more outgoing longwave radiation
  2. Water vapour is the original source of solar energy
  3. Water vapour always raises Earth’s albedo to one hundred percent
  4. Water vapour changes Earth’s shape
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  1. The balance applies to the total amount, while energy can still be unevenly distributed between regions.
  2. Energy cannot be transferred when the total is balanced.
  3. A balanced heat budget means there is no energy.
  4. The Sun stops supplying energy when the budget is balanced.
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  1. For a while after maximum insolation, the surface continues gaining more energy than it loses.
  2. The Sun first appears after noon.
  3. Earth does not emit radiation during the day.
  4. Clouds stop time from passing.
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  1. Because it includes conduction, convection, and latent heat transfers as well as radiation
  2. Because it does not include energy
  3. Because it is only an account of rainfall
  4. Because it describes only ocean tides
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  1. Their altitude, thickness, and radiative properties differ
  2. High clouds do not interact with energy
  3. Low clouds are made only of soil
  4. All clouds have exactly the same effect
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  1. It indicates how effectively the surface emits longwave radiation
  2. It indicates how large the Sun is
  3. It reduces the height of the atmosphere
  4. It stops Earth from revolving
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  1. Their surface types, moisture, cloud cover, altitude, and influence from the sea may differ
  2. Everything is identical at the same latitude
  3. The Sun shines at only one of the places
  4. Earth's shape keeps changing from place to place
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  1. High albedo reflects more incoming sunlight, while counter-radiation reduces the surface’s net longwave heat loss
  2. Both effects remove all energy from the area
  3. Both effects only change wind direction
  4. Neither effect has any connection with temperature

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