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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 2 · 25 questions

TOPIC PRACTICE

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  1. Because solar heating and atmospheric convection vary. (सौर ताप और वायुमंडलीय संवहन में अंतर के कारण।)
  2. Because of Earth's metallic content. (पृथ्वी में धातुओं की मात्रा के कारण।)
  3. Because of ocean salinity. (महासागरीय लवणता के कारण।)
  4. Because of gases in the exosphere. (बहिर्मंडल की गैसों के कारण।)
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  1. Ordinary rainfall
  2. Evaporation from rivers
  3. The effect of solar radiation
  4. Ocean waves
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  1. Temperature remains the same in both
  2. Temperature decreases in both
  3. Temperature rises in the troposphere and falls in the stratosphere
  4. Temperature falls in the troposphere and rises in the stratosphere
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  1. It affects air stability and convection
  2. It ends the exosphere
  3. It forms the oceans
  4. It completely destroys ozone
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  1. Temperature increases with height
  2. Pressure increases with height
  3. Clouds increase with height
  4. Rainfall increases with height
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  1. Clouds and rainfall
  2. Air near the surface
  3. Ionization and very high temperature
  4. Agricultural soil
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  1. Rainfall increases in the mesosphere
  2. Temperature generally increases with height in the stratosphere
  3. Clouds form in the exosphere
  4. The troposphere ends
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  1. Greater ocean salinity
  2. Less heating and weaker convection
  3. Complete absence of ozone
  4. Pressure from the exosphere
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  1. Humidity, cloud cover, and local heating conditions vary
  2. The thickness of the exosphere changes it
  3. The colour of ozone changes it
  4. Only the number of meteors changes it
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  1. Because the few particles absorb high-energy solar radiation
  2. Because water vapour is dense there
  3. Because clouds cover the surface there
  4. Because rain produces heat there
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  1. It helps mix heat and moisture vertically
  2. It completely destroys the ozone layer
  3. It makes the exosphere denser
  4. It stops meteors from entering the atmosphere
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  1. Temperature generally rises with height there, increasing atmospheric stability
  2. Strong storms form there continuously
  3. Water vapour is most abundant there
  4. The Earth's surface heats it directly
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  1. Warmer, less-dense air lies above cooler, denser air, creating a stable arrangement
  2. Water vapour suddenly becomes very abundant there
  3. Air weighs more there than at sea level
  4. Gravity stops acting there
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  1. Heating is limited and radiative cooling contributes to the cold upper mesosphere
  2. Continuous rainfall occurs there because of abundant water vapour
  3. Sunlight does not reach the mesopause at all
  4. Heat from Earth’s surface travels directly there
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  1. Because it is near sea level
  2. Because temperatures are very low at the top of the mesosphere
  3. Because ozone produces the most heat there
  4. Because all clouds collect there
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  1. Because the availability of solar radiation changes
  2. Because ocean salinity changes
  3. Because the groundwater level changes
  4. Because the gradient of a river changes
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  1. Thermosphere
  2. Troposphere
  3. Lower troposphere
  4. Surface boundary layer
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  1. From mesosphere to thermosphere
  2. From troposphere to stratosphere
  3. From exosphere to troposphere
  4. From surface to ocean
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  1. Stratosphere
  2. Troposphere
  3. Thermosphere
  4. Mesosphere
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  1. Troposphere
  2. Exosphere
  3. Mesosphere
  4. Thermosphere
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  1. Stratosphere
  2. Troposphere
  3. Mesosphere
  4. Exosphere
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  1. Temperature increases with height, making the air stable
  2. Surface friction is very strong throughout the stratosphere
  3. Rain clouds continuously rise upward
  4. Air pressure increases with height
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  1. Ozone absorbs ultraviolet radiation in the upper stratosphere.
  2. Rain clouds form in the mesosphere.
  3. Cold air descends from the exosphere.
  4. Air pressure becomes zero in the troposphere.
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  1. Temperature increases upward, creating stable stratification.
  2. Water vapour travels there directly from the surface.
  3. Pressure remains equal at every height.
  4. Winds stop completely there.
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  1. Absorption of ultraviolet radiation by ozone
  2. Evaporation of tropospheric rainfall
  3. Condensation of exospheric dust
  4. Freezing of mesospheric meteors

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