Solar Radiation, Heat Balance and Temperature
Class 11 Geography · Fundamentals of Physical Geography · Chapter 8
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View allCBSE Class 11 · Geography
Earth's interior + plates: Unit II, 9 marks- Marks booster + cheatsheet: key concepts in 2 lines each, common traps
- 8 marks: Climate unit, Ch 7–10
- 5 marks: map work, covered
- 4 marks: ocean data as charts, Unit V
- Heat budget and five air layers as charts
- Common traps, corrected
CBSE Class 11 · Geography
Physiography + Drainage: Unit II, 13 marks- Marks booster + cheatsheet: key concepts in 2 lines each, common traps
- 12 marks: Climate, Vegetation (Unit III)
- Full CBSE map-work list, chapter by chapter
- Indus, Ganga, Brahmaputra river systems
- Monsoon mechanism, onset and four seasons
- Common traps, corrected
CBSE Class 11 · Geography
Projections, Remote Sensing: 5 marks each- Marks booster + cheatsheet: key concepts in 2 lines each
- 4 marks: Map Scale, conversions worked
- 4 marks: Latitude, Longitude and Time
- 4 marks: Topographical Maps, contours
- 5 marks: practical file and viva
- Conical and Mercator's construction steps
Summary
The earth receives almost all its energy from the sun as short-wave incoming solar radiation, called insolation; on average the top of the atmosphere receives 1.94 calories per sq cm per minute. Because the earth is a geoid, the sun's rays fall obliquely and only a small portion is intercepted. The earth is farthest from the sun (aphelion) on 4 July and nearest (perihelion) on 3 January. Insolation varies with the rotation of the earth, the angle of the sun's rays, the length of day, atmospheric transparency and configuration of land. The atmosphere is heated by conduction, convection, advection and terrestrial radiation. The heat budget keeps the earth's temperature constant: of 100 units of insolation, 35 are reflected (the albedo), 65 are absorbed and ultimately returned, balancing the total received. There is a surplus of net radiation between 40°N and 40°S and a deficit near the poles, redistributed pole-ward. Temperature is controlled by latitude, altitude (normal lapse rate of 6.5°C per 1,000 m), distance from the sea, air masses and ocean currents. Temperature distribution is shown by isotherms, and at times the normal lapse rate is reversed in an inversion of temperature.







