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Subjects

Geography

Heating and cooling of the atmosphere

In this Class 11 Geography topic, students learn how the atmosphere is heated and cooled through incoming solar radiation and outgoing terrestrial radiation. The lesson explains Earth’s heat balance and the roles of conduction, convection, advection, and latent heat in transferring energy through the atmosphere. Students also examine how land and water surfaces, cloud cover, humidity, and atmospheric circulation influence temperature patterns and help produce differences between places and times.

Medium · Level 7 · 25 questions

TOPIC PRACTICE

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25 questions

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  1. River erosion
  2. Expansion or compression of air due to pressure change
  3. Only surface colour
  4. Lunar eclipse
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  1. Moon tide river erosion
  2. Longitude time zone population
  3. Solar energy absorption terrestrial radiation atmospheric heating heat loss
  4. Sea salinity earthquake mountain
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  1. Because wind forms only from the Moon
  2. Because temperature has no relation with pressure
  3. Because air has no density
  4. Because temperature difference creates pressure difference
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  1. Because an open dry surface can lose more radiational heat
  2. Because grass makes the Sun shine at night
  3. Because dry soil has no atmosphere
  4. Because grass creates sea
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  1. Energy will become completely double
  2. Dust can reduce energy through scattering and absorption
  3. Dust will increase day length
  4. Energy will come only from the Moon
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  1. Because heat comes from the surface through terrestrial radiation and conduction
  2. Because the upper atmosphere is always sea
  3. Because the surface blocks the Sun
  4. Because lower air has no gas
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  1. Wind increases air mixing and can reduce extreme cooling near the surface
  2. Wind makes the Sun rise at night
  3. Wind changes the solar constant
  4. Wind turns land into sea
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  1. Clouds bring the Sun closer to Earth
  2. Clouds make air zero
  3. Clouds reflect and block part of incoming solar radiation
  4. Clouds double the length of day
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  1. The surface absorbs solar energy and emits terrestrial radiation
  2. The surface receives energy from the Moon
  3. The surface removes all clouds
  4. The surface removes air
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  1. Upper ionosphere
  2. Lower air touching the surface
  3. Mid ocean
  4. Outer space
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  1. Reflection
  2. Albedo
  3. Convection
  4. Tide
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  1. When the surface changes colour
  2. When the Moon is full
  3. When river flow is slow
  4. When wind brings air of different temperature
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  1. The Sun gives shortwave and Earth emits longwave radiation
  2. The Sun gives only longwave radiation
  3. Earth gives only shortwave radiation
  4. Both are sound waves
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  1. Dense cloudy night
  2. Clear calm night
  3. Rainy day
  4. Sea storm
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  1. Create terrestrial radiation by day and increase Sun at night
  2. Stop wind by day and dry oceans at night
  3. Reflect solar radiation by day and trap longwave radiation at night
  4. Have no effect by day or night
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  1. It moves the Sun away
  2. It makes air pressure zero
  3. It removes albedo
  4. It absorbs latent heat
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  1. Both always have the same colour
  2. Their heat capacities are different
  3. Sunlight does not fall on both
  4. Both have no atmosphere
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  1. Complete absence of land
  2. Greater influence of the Moon
  3. Slow heating and cooling of the sea
  4. Zero density of air
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  1. Because the sea is near
  2. Because the Sun does not come there
  3. Because wind does not blow
  4. Because land heats and cools quickly
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  1. General decrease of temperature with height
  2. Salinity of sea
  3. River bend
  4. Shape of the Moon
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  1. Normal decrease of temperature with height
  2. Increase of temperature with height
  3. Sea temperature becoming zero
  4. Complete absence of air
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  1. The Sun heats the valley
  2. Sea breeze enters the valley
  3. Cold dense air collects below
  4. River stops evaporation
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  1. Because the Sun sets at noon
  2. Because the Moon increases temperature
  3. Because albedo suddenly becomes zero
  4. Because energy gain remains greater than loss for some time
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  1. Heat loss by terrestrial radiation throughout the night
  2. Stronger heating by the Sun
  3. Greater evaporation of water
  4. Increase in day length
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  1. They remove all clouds
  2. They absorb part of terrestrial radiation
  3. They change Earth's axis
  4. They lengthen the day

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