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Subjects

Geography

The heat budget of the earth

पृथ्वी का ऊष्मा बजट

Class 11 Geography explores the heat budget of the Earth as the balance between incoming solar radiation and outgoing terrestrial radiation. Students learn how the atmosphere, land, oceans, clouds, and ice reflect, absorb, store, and redistribute heat, and why the Earth’s average temperature remains broadly stable. The topic connects this balance with the greenhouse effect, latitudinal differences in heating, and the movement of heat through the atmosphere and oceans.

TOPIC PRACTICE

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Up to 25 questions from this page. Select your focus, then start.

25 questions

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Hard · Level 3
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  1. Because reflection emission moisture and heat transfer also affect it
  2. Because incoming solar energy has no effect
  3. Because temperature is decided only by population
  4. Because surface never receives energy
Hard · Level 3
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  1. It is the balance of energy input transformation transfer and output in the Earth atmosphere system
  2. It is only a list of Sun's distance
  3. It is only counting clouds
  4. It is only ocean depth
Hard · Level 3
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  1. Absorbed energy will decrease by five units
  2. Absorbed energy will increase by five units
  3. Absorbed energy will remain same
  4. Absorbed energy will become hundred units
Hard · Level 3
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  1. Surface absorption may increase
  2. Surface absorption will become zero
  3. Solar radiation will arrive as longwave
  4. Terrestrial radiation will stop
Hard · Level 3
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  1. Sixty five units of outgoing longwave energy
  2. Only thirty five units of reflected energy
  3. Only fifty one units of solar energy
  4. Fourteen units of surface reflection
Hard · Level 3
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  1. Seventeen units
  2. Forty eight units
  3. Thirty five units
  4. Fifty one units
Hard · Level 3
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  1. Atmospheric window
  2. Solar constant
  3. Water cycle
  4. Ocean salinity
Hard · Level 3
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  1. It will decrease
  2. It will increase
  3. It will become shortwave
  4. It will be fully reflected
Hard · Level 3
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  1. Increase in snow and cloud cover
  2. Increase in dark urban surfaces
  3. Complete removal of forests exposing dark soil
  4. Darkening of ocean surface
Hard · Level 3
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  1. Absorption may increase causing further warming
  2. Reflection will increase and surface will cool immediately
  3. Solar energy will stop
  4. Atmospheric window will disappear
Hard · Level 3
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  1. They can reflect shortwave by day and counter radiate longwave at night
  2. They only destroy energy
  3. They only reduce surface albedo
  4. They only warm oceans
Hard · Level 3
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  1. Daily temperature range may decrease
  2. Daily temperature range will always double
  3. Both day and night will be equally very cold
  4. Solar energy will increase at night
Hard · Level 3
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  1. Strong sunshine low albedo and fewer clouds
  2. Long clear night and dry air
  3. Snow surface and oblique sun rays
  4. Thick daytime cloud and high reflection
Hard · Level 3
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  1. Clear night and strong terrestrial radiation
  2. Strong noon sunshine and dark surface
  3. Fewer clouds and high solar angle
  4. Clear day near equator
Hard · Level 3
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  1. Atmosphere oceans and terrestrial radiation remove extra energy
  2. Solar energy never comes there
  3. Albedo is always hundred percent
  4. Earth does not absorb energy there
Hard · Level 3
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  1. Heat is transported from low latitudes
  2. The Sun shines most directly there
  3. There is no outgoing energy there
  4. Snow absorbs all energy
Hard · Level 3
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  1. Latitudinal heat balance
  2. Only water salinity balance
  3. Only mountain balance
  4. Only soil particle balance
Hard · Level 3
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  1. It redistributes energy through air masses
  2. It stops Earth from receiving energy
  3. It permanently makes albedo zero
  4. It prevents terrestrial radiation from forming
Hard · Level 3
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  1. Absorbed energy remains continuously greater than outgoing energy
  2. Reflected energy is greater than absorbed energy
  3. Outgoing energy is greater than incoming energy
  4. Solar input becomes zero
Hard · Level 3
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  1. It can lower the average temperature
  2. It can raise the average temperature
  3. It can keep the average temperature constant
  4. It can increase Earth’s rotational speed
Hard · Level 3
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  1. Outgoing longwave terrestrial radiation
  2. Creation of incoming visible solar energy
  3. Ocean tides
  4. Mountain building energy
Hard · Level 3
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  1. Escape of longwave energy may increase
  2. Solar energy will increase at night
  3. Surface reflection will stop
  4. Earths energy gain will become zero
Hard · Level 3
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  1. A warmer surface radiates more energy
  2. A warmer surface stops radiation
  3. A warmer surface only receives shortwave
  4. A warmer surface cools the Sun
Hard · Level 3
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  1. It absorbs shortwave solar energy and emits longwave terrestrial energy
  2. It converts longwave solar energy into shortwave
  3. It converts all energy into sound
  4. It does not convert energy
Hard · Level 3
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  1. Possibility of energy surplus will increase
  2. Energy deficit will be certain
  3. Reflection will be hundred percent
  4. Solar energy will be zero

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