Atmosphere – Solar Radiations, Heat Budget, Temperature Inversion

Atmosphere – Solar Radiations, Heat Budget, Temperature Inversion

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Atmosphere – Solar Radiations, Heat Budget, Temperature Inversion

Solar Radiations

  • Maximum at equator & min. at poles (Due to earth’s inclination & its spherical shape, Sunrays fall perpendicular to equator, with inclination increasing from equator to poles)
  • Larger the thickness / wideness of atmosphere, greater the scattering, reflection & absorption by the atmosphere, reducing the intensity of insolation on earth’s surface
  • As beam of sunrays falls perpendicular to equator, hence if sunrays cross 1 unit of atmosphere here then they have to cross almost 44.7 units at poles
  • That is why Insolation received per unit area is max at equator & min at poles

Specific Heat

  • Heat capacity or specific heat of water is 5 times that of earth surface
  • Which means same amount of heat will heat earth’s surface 5 times than that of water of same mass & vice-a-versa in case heat is withdrawn
  • Hence land surface heats & cool more rapidly than water surface
  • Specific Heat [arr] Energy required to raise the temperature of 1 gm of substance by 1*C
  • Rate of Heating differ between Water & Land because water is transparent to sunrays & is always in motion
  • Hence heat is absorbed more slowly as absorbed heat is distributed over a great depth & area.

Heat Budget

  • Earth maintains its temp. as amount of heat received by it in form of insolation = Amount of heat radiated by it through terrestrial radiation.
  • Gain & loss of heat or balance of heat (Received & Emitted) is known as heat budget

Heat Received

  • Total Solar Radiations [arr] 100%
  • Returned back to atmosphere in short wave form [arr] 35% (Mainly from reflection & scattering from clouds, dust particles & from earth surface)
  • Absorbed by atmosphere (mostly water vapour + Dust + Gases) [arr] 14%
  • Available to earth [arr] 51% (34% from direct sunlight & 17% from scattered radiations) [arr] Hence only 65% of total insolation is available for heating atmosphere.

Heat Budget

Note [arr] Clouds act generally as mirror, reflects sunlight in different directions rather than absorbing it (Reflected sunlight is permanently lost to earth)

Heat Radiated

  • Returned as long wave radiation form earth [arr] 51 %
  • 17 % radiated from earth surface
  • 34 % absorbed by atmosphere (19 % + 9 % + 6 %)
  • Now, 48 % (34 % + 14 %) absorbed by atmosphere is radiated to space by atmosphere.

Hence, Total Heat Received = Total Heat Radiated


Temperature Variation

  • Under normal circumstances temperature decreases from equator to poles & each latitude has its own temp.
  • But other factors such as altitude, oceanic currents, prevailing winds etc. also affect the temp. of a place.
  • Hence, there lies a difference b/w temp. of a place & mean temp. of its parallel [arr] Known as temperature / thermal anomaly

Temperature Variation on earth

  • If Expected temp. of a place (latitude) minus actual temp. of that place is negative then it is called negative anomaly & if positive then positive anomaly
  • Due to more land area in northern hemisphere & more water area in southern hemisphere, largest of anomalies are found in N – Hemisphere & smallest in S – Hemisphere

Isotherms

  • Imaginary lines joining places having equal temperatures, reduced to sea level to eliminate the effect of altitude
  • Runs almost parallel to latitudes but modified somewhat due to influence of land & sea
  • At any latitude, temperature over land mass is higher in summer & lower in winters compared to the temp. over sea
  • Hence isotherms while crossing from landmass to oceans bend a little & vice a versa
  • In January, there is winter in N – Hemisphere & summer in S – Hemisphere, means air over oceans is warmer than that over land masses in N – Hemisphere
  • Hence isotherms bend equatorward while crossing the landmasses & polewards while crossing the oceans (Vice a versa in summers in N – Hemisphere) + Same logic for S – Hemisphere
  • More water in S hemisphere results in uniform temp. mostly, hence less bends in isotherms [arr] Trend is more clear here than at N – Hemisphere
  • Distance b/w isotherms represents rate of change of temp., hence closely spaced isotherms indicate rapid change in temp. & vice versa.

Diurnal/Daily Range of Temperature

  • Difference b/w max. temp. during day & min. during night;
  • Sufficiently high at equator & gradually decreases towards poles
  • Minimum near sea cost due to moderating effect of sea;
  • Deserts have high diurnal range of temp. as sand absorbs & radiates quicker than land surface
  • Cloud cover reduces daily range of temp. as it obstructs incoming radiations during day & outgoing radiations during night

Annual Range of Temperature

  • Difference b/w average temp. of hottest & coldest month of the year
  • Minimum at equator & max at poles

Temperature Inversion

  • Under normal conditions, temp. of atmosphere fall with altitude
  • But there are some special conditions under which temp. increases instead of decreasing with height.
  • Means air near earth surface is cooler than that of higher place
  • Factors which favour this condition are long nights, Clear sky, Stable weather, Dry air & Ice cover.

Air Drainage Temperature Inversion

  • In mountain valleys, during long winter nights, air on higher slopes cool down quickly & become dense
  • Hence move down the slope & settle down at valley bottom, pushing comparatively warmer air up
  • Sometimes temp. at valley bottom falls below freezing point & air above at higher altitude remains comparatively warm,
  • As a result, trees at lower slopes are mostly frost bitten than that of at higher slopes
  • Houses & farms in mountain valley are generally situated along the upper slopes avoiding cold & foggy valley bottoms
  • Air pollutants such as dust, smoke etc. do not disperse at valley bottom due to this reason

Air Drainage Temperature inversion

Radiation Temperature Inversion

  • In areas, where there is rapid cooling of earth surface due to intense radiation from earth’s surface
  • As a result air close to earth surface becomes cooler than air at higher elevation
  • Generally occurs in winters

Radiation Temperature Inversion

Advection Temperature Inversion

  • In areas, where warmer air blows over colder surface
  • Example [arr] Snow covered area

Advection Temperature Inversion

Frontal Temperature Inversion

  • When warm air mass rises over cold air mass
  • Generally, occurs in mid latitudes where cold polar air mixes with warm subtropical air mass
  • Lots of fog is generated

Frontal Temperature Inversion

3 comments
  1. Hello,
    Your content is really good. I was referring NCERT text books till now. But as came by you website, I felt I can understand your notes easily and better than NCERT as you have mentioned everything point wise and also with more pictures. I want to know whether I can replace my NCERT and read your notes only. Please do reply.

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