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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.

Expert · Level 2 · 25 questions

TOPIC PRACTICE

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  1. Strong convection and higher sensible heat
  2. Complete absence of radiation
  3. Permanent temperature inversion
  4. Sea-like evaporation effect
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  1. Surface cover changes energy partitioning
  2. Latitude becomes different at both places
  3. Concrete makes air invisible
  4. Forest changes the solar constant
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  1. Energy is used in transpiration and evaporation
  2. Irrigation increases solar altitude
  3. Grass does not stop longwave radiation
  4. Solar energy does not reach dry land
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  1. Daytime heating and nighttime radiational cooling of slopes
  2. Daily change in ocean salinity
  3. Daily change in Earth orbit
  4. Descent of ozone layer to surface
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  1. Clear calm long night and pooling of cold air on valley floor
  2. Strong daytime wind and intense convection
  3. Thick daytime cloud and rainfall
  4. Warm current on sea surface
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  1. Atmosphere absorbs longwave energy more effectively than shortwave energy
  2. Longwave energy comes directly from the Sun
  3. Land does not emit longwave energy
  4. Atmosphere reflects all waves completely
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  1. Water vapour varies strongly with local and short-term humidity
  2. Water vapour absorbs no longwave energy
  3. Water vapour occurs only in the stratosphere
  4. Water vapour always remains as ice
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  1. They reduce shortwave energy by day and trap longwave energy at night
  2. They only increase solar energy both day and night
  3. They make Earth a Sun at night
  4. They remove the mass of air
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  1. The surface is gaining energy and tends to warm
  2. The surface is only losing energy
  3. Solar radiation is absent
  4. The atmosphere has completely cooled
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  1. Radiational cooling
  2. Intense solar heating
  3. Permanent noon
  4. Boiling of seawater
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  1. Shade and transpiration redistribute surface energy
  2. Vegetation reduces the distance to the Sun
  3. Solar energy does not reach rocky land
  4. Vegetation does not produce terrestrial radiation
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  1. Strong surface heating and sufficient moisture
  2. Surface remaining below freezing continuously
  3. Calm dry and very cold night
  4. Complete stability by warm layer aloft
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  1. Air temperature approaches the dew point
  2. Solar altitude suddenly increases
  3. Air pressure disappears completely
  4. Solar energy comes out of the ground
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  1. Clear calm night and enough moisture near surface
  2. Strong dry hot wind
  3. Intense noon convection
  4. Dust-free upper stratosphere
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  1. It mixes the cold surface layer with air above
  2. It creates solar energy at night
  3. It turns water vapour into solid rock
  4. It always increases terrestrial radiation
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  1. Warm moist air flows over a cold surface
  2. Cold dry air stays over a hot desert
  3. Hot dry air moves over high mountain
  4. Surface and air are equally warm
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  1. It starts heating or cooling of the first air layer touching the surface
  2. It directly heats the whole troposphere
  3. It creates solar energy
  4. It occurs only in deep oceans
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  1. Entry of a warm or cold air mass into a region
  2. Direct contact heating from surface to air
  3. Rising column of warm air
  4. Surface radiation on a clear night
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  1. Immediate air heating may decrease
  2. Air temperature will immediately rise greatly
  3. Water vapour will vanish
  4. Solar angle will change
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  1. Surface may become relatively cooler due to increased evaporation
  2. Surface will always become hotter
  3. Terrestrial radiation will completely stop
  4. Albedo will always become zero
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  1. Surface air density decreases and buoyancy increases
  2. Gravity disappears at the surface
  3. Water vapour changes into nitrogen
  4. Solar radiation becomes lunar radiation
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  1. Surface heating then convection then cooling then condensation
  2. Condensation then solar heating then creation of surface
  3. Terrestrial radiation then drying of sea then cloud
  4. Cold surface then sinking air then strong sunshine
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  1. Convection
  2. Reflection
  3. Latitude change
  4. Permanent glacier movement
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  1. When evaporation is low and water vapour is high
  2. When air is completely dry and cold
  3. When snow albedo is very high
  4. When strong cold wind blows
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  1. Land heats quickly and lifts air while sea remains relatively cooler
  2. Sea always lifts the air
  3. There is no atmosphere over land
  4. Sea temperature is zero every day

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