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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.

Hard · Level 2 · 25 questions

TOPIC PRACTICE

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  1. Land heats faster than sea and forms low pressure
  2. Sea heats faster than land and forms high pressure
  3. Solar radiation is stronger at night
  4. Water temperature always remains zero
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  1. Land cools faster than sea and forms high pressure
  2. The sea freezes at night
  3. Land produces solar energy at night
  4. Sea pressure is always zero
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  1. Slope air heats by insolation and moves upslope
  2. Melting snow at night pushes air downward
  3. Pressure in valleys always remains equal
  4. Radiation does not occur on slopes
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  1. Slope air becomes cold and dense by radiational cooling
  2. The Sun heats slopes at night
  3. Valley air disappears completely
  4. Air can move only toward the sea
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  1. Low sun angle spreads energy over a larger area
  2. The Moon cools the day
  3. Earth stops producing solar radiation
  4. Air destroys heat
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  1. Oblique rays spread over a larger area and travel through a longer path in the atmosphere
  2. The atmosphere is completely absent at high latitudes
  3. During long days, the Sun does not rise above the horizon at high latitudes
  4. The Earth does not emit longwave radiation at high latitudes
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  1. The main heat source is the Earth’s surface
  2. The Sun becomes weak at height
  3. Upper air has no gas
  4. Gravity destroys heat
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  1. Normal lapse rate is environmental temperature change, while adiabatic rate relates to moving air parcels
  2. Both describe only ocean temperature
  3. Both are always equal and fixed
  4. Neither has any relation to radiation
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  1. Warm, less-dense air can rise rapidly
  2. Rising air becomes cooler and denser than the surrounding air
  3. Temperature begins to increase with height near the surface
  4. Cold air aloft prevents mixing with warm lower air
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  1. Cold dense air below and warmer air above resist uplift
  2. Warm air sinks and becomes lighter
  3. Conduction becomes very fast
  4. Solar radiation goes inside Earth
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  1. It prevents vertical mixing and traps cold, moist air near the ground
  2. It produces strong convection in the upper atmosphere and lifts the fog upward
  3. It rapidly warms the surface and evaporates the water droplets
  4. It completely removes water vapour from the lower air
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  1. Latent heat is released during condensation, slightly reducing the cooling of the air
  2. Latent heat is absorbed through evaporation, causing the air to cool rapidly
  3. Dew formation has no effect on the temperature of nearby air
  4. Dew formation immediately lowers the air temperature below the freezing point
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  1. Latent heat for melting is taken from surroundings
  2. Melting snow produces fire
  3. Snow completely stops the Sun
  4. Melting needs no energy
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  1. It expands and cools adiabatically while rising
  2. Air expands while descending
  3. Mountains destroy solar radiation
  4. Rain always heats air
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  1. Compression during descent causes adiabatic heating
  2. Solar radiation does not reach a rain-shadow area
  3. Descending air cools and condenses
  4. Mountains create water vapour on the windward slope
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  1. Air is a poor conductor of heat
  2. Air has no molecules
  3. Conduction occurs only in oceans
  4. Conduction comes from the Sun
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  1. Rising warm moist air cools and condenses
  2. Sinking cold air always forms clouds
  3. Clouds form only by conduction
  4. Terrestrial radiation destroys water vapour
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  1. Direct heat transfer between surface and air
  2. Hidden heat used in water vapour formation
  3. Ocean salinity
  4. Earth’s magnetic field
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  1. Energy is used in evaporation instead of raising temperature
  2. Energy is completely destroyed
  3. Evaporation occurs only at night
  4. Latent heat exists only in rocks
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  1. Water vapour absorbs terrestrial radiation and increases downward counter-radiation
  2. Humid air stores more solar energy during the day and releases it at night as solar radiation
  3. Desert sand absorbs more terrestrial radiation at night than water vapour
  4. High humidity causes Earth to stop emitting radiation towards space at night
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  1. Concrete has less evapotranspiration and more heat storage
  2. Grass increases solar energy
  3. Concrete has no thermal property
  4. Grass emits no longwave radiation
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  1. The minimum temperature will remain relatively higher
  2. The minimum temperature will decrease further
  3. The minimum temperature will not change
  4. The minimum temperature will always fall below freezing point
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  1. More solar radiation reaches the surface, so heating may increase
  2. The surface receives no energy
  3. Conduction completely stops
  4. Evaporation becomes impossible
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  1. The stable layer suppresses vertical mixing and dispersion of pollutants
  2. The stable layer increases surface wind speed and carries pollutants away
  3. A cooling surface immediately converts pollutant particles into water vapour
  4. In a stable layer, air aloft rapidly warms and destroys pollutants
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  1. High sun angle heats the surface strongly and lifts air
  2. Nights are always long there
  3. There is no atmosphere there
  4. Sun rays heat only clouds

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