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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 9 · 19 questions

TOPIC PRACTICE

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Up to 19 questions from this page. Select your focus, then start.

19 questions

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  1. Evaporation in wet soil uses heat
  2. Sunlight does not fall on dry soil
  3. Wet soil has no temperature
  4. Dry soil is always ice
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  1. Wind makes the Sun shine
  2. Wind increases air mixing and weakens the cold surface layer
  3. Wind changes the solar constant
  4. Wind creates sea
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  1. Heating of slopes and nearby air becoming lighter
  2. Moon pulling the slopes
  3. Sea waves reaching the mountain
  4. Permanence of snow
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  1. Radiational cooling of slopes makes air cold and heavy
  2. The Sun heats slopes at night
  3. The sea changes into mountain
  4. Air density becomes zero
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  1. Change in air temperature due to pressure change without heat exchange
  2. Temperature change by surface colour
  3. Temperature change by Sun distance
  4. Temperature change by Moon brightness
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  1. Absorption of solar energy then terrestrial radiation then atmospheric heating then heat loss
  2. Moon then tide then river
  3. River then mountain then rainfall
  4. Longitude then time zone then population
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  1. They create temperature and pressure differences that move air
  2. They create lunar eclipses
  3. They change names of rivers
  4. They remove the atmosphere
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  1. Because latent heat is absorbed during melting
  2. Because snow doubles the Sun
  3. Because melting removes air pressure
  4. Because snow increases day length
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  1. Water vapour absorbs some of the longwave radiation emitted by Earth's surface.
  2. Water vapour makes the Sun larger at night.
  3. Water vapour stops Earth from orbiting the Sun.
  4. Water vapour reduces the solar constant.
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  1. Low water vapour and often clear skies allow strong daytime heating and rapid radiative cooling at night
  2. Thick clouds trap heat equally throughout the day and night
  3. The nearby sea has a high heat capacity
  4. Snow cover raises the surface albedo
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  1. There is less water vapour and cloud cover to absorb outgoing longwave radiation and emit it back toward the surface
  2. The Sun moves much farther away at night
  3. The surface stops emitting radiation at night
  4. Oceans create all the heat in the atmosphere
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  1. Paved surfaces store heat during the day and release it gradually at night
  2. The Sun shines over the city at night
  3. Terrestrial radiation does not occur in cities
  4. Clouds form only over cities
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  1. Clear skies allow strong solar heating by day, while dry air allows terrestrial heat to escape readily at night.
  2. The Sun is absent during the day, while clouds form every night.
  3. Sand does not emit terrestrial radiation.
  4. Water vapour completely blocks all longwave radiation.
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  1. Water has a high heat capacity, and mixing spreads heat through a larger volume.
  2. Sand reflects all incoming sunlight.
  3. Coastal areas have no atmosphere.
  4. The Sun is cooler over coastal areas.
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  1. There is no incoming solar radiation at night, but downward atmospheric longwave radiation affects the surface’s heat loss
  2. The Sun gives off more heat at night
  3. The surface stops emitting energy at night
  4. The oceans disappear at night
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  1. It need not increase by the same amount as surface emission, because the atmosphere can re-emit absorbed energy upward and downward
  2. It will always double
  3. It must remain zero
  4. The longwave radiation will become solar shortwave radiation
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  1. Water vapour absorbs outgoing infrared radiation and helps retain heat near the surface.
  2. Water vapour makes the Sun shine more brightly during the night.
  3. Water vapour increases the total mass of the Earth.
  4. Water vapour changes the atmosphere into a solid.
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  1. Some solar energy may be reflected
  2. More sunlight may reach Earth's surface
  3. Water vapour may completely disappear from the atmosphere
  4. All chances of rainfall may end
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  1. The direction of radiation may change
  2. The total mass of the atmosphere may vanish on its own
  3. Ocean salinity may immediately become zero
  4. The height of mountains may suddenly increase

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