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☀️Solar Radiation & Temperature: Energy for Crop Growth

Heat transfer, solar constant, albedo, light spectrum, PAR, light compensation and saturation points, cardinal temperatures, heat and cold injuries — with agricultural examples and exam tips

Why Solar Radiation Matters to Farmers

In the previous lesson, we covered monsoon systems and precipitation — the SW and NE monsoons, types of rainfall, and how moisture reaches crops. Now we examine the other side of the energy equation: solar radiation and temperature, which together determine how efficiently crops use that moisture.

A sugarcane farmer in Maharashtra knows that his crop needs intense sunlight to convert solar energy into sugar. A betel vine grower in West Bengal deliberately provides shade because his crop wilts under direct sun. Every crop has specific light and temperature requirements — understanding solar radiation is the starting point for matching crops to environments.

This lesson covers:

  1. Heat transfer — conduction, convection, radiation, and latent heat
  2. Solar constant and albedo — how much energy arrives and how much is reflected
  3. Earth’s energy budget — the 100% incoming radiation balance
  4. Light spectrum and PAR — which wavelengths drive photosynthesis
  5. Photoperiodism — short-day, long-day, and day-neutral crops
  6. Temperature and crop growth — cardinal temperatures, heat injuries, and cold injuries
  7. Oasis effect — local cooling from vegetation

All topics are high-yield for IBPS AFO, NABARD, and ICAR-JRF exams.


Transfer of Heat

All matter above absolute zero emits energy. Three processes transfer heat:

ProcessMechanismExampleAgricultural Relevance
ConductionHeat flows through matter without movement of the substanceHeat passing through an iron rodSoil heat transfer — surface warming reaches roots by conduction
ConvectionHeat transfer through actual movement of moleculesBoiling water in a beakerPredominant form of energy transfer on earth; drives all weather processes affecting crops
RadiationEnergy transfer without any material mediumSun’s energy reaching earth through spaceSolar radiation reaching crop canopies; basis of photosynthesis

TIP

Exam mnemonic — “CCR”: Conduction = Contact, Convection = Circulation (movement), Radiation = Remote (no medium needed). Convection is the most important for weather.


Latent Heat

When solar radiation hits a surface, it is partly absorbed, partly reflected, and partly transmitted.

Latent heat is the energy required to change a substance to a higher state of matter (solid → liquid → gas). The same energy is released in the reverse process.

Agricultural example: When water evaporates from a rice paddy field, it absorbs latent heat from the surroundings, cooling the field. When this moisture condenses into clouds, latent heat is released — this is why the wet adiabatic lapse rate (6°C/km) is lower than the dry rate (10°C/km).


Solar Constant

Solar constant is the energy received on a unit area at the outermost boundary of the earth’s atmosphere, held perpendicular to the sun’s direction, at the mean distance between the sun and the earth.

IMPORTANT

Solar constant = 1.94 cal/cm²/min (also called 1 Langley per minute)

Agricultural significance: The solar constant sets the upper limit of energy available for photosynthesis. Only about 1% of incoming light energy is converted into biochemical energy by crops, and the most efficient crop (sugarcane) uses only 10–12% of total solar energy.


Albedo

Albedo is the percentage of reflected radiation to the incident radiation. A high albedo means more reflection and less absorption.

Albedo Values of Different Surfaces

SurfaceAlbedo (%)SurfaceAlbedo (%)
Ice90 (highest)Wheat23–25
Indian soil35Rice12
Average of earth30Potato19
Meadows10–20Pearl Millet (Bajra)24
Ploughed soil14–17Moong26
Black dry soil14Crop plants (general)15–25
Black moist soil08 (lowest)Lucerne23–32
Grey dry soil25–30Grey moist soil10–12

TIP

Exam fact: Ice = highest albedo (90%). Black moist soil = lowest (8%). Earth’s average = 30%. Most soils have albedo of 0.10 to 0.15.

Agricultural significance: A freshly ploughed dark field (low albedo) absorbs more heat and warms up faster, promoting early germination. Mulching with light-coloured straw (higher albedo) keeps soil cooler — useful in summer vegetable cultivation.


Earth’s Energy Budget

Not all solar energy reaching Earth is available to crops. The atmosphere, clouds, and surface all interact with incoming radiation. Of the total incoming solar energy (100%):

Incoming Radiation

ComponentPercentage
Absorbed by land and oceans51%
Reflected by clouds20%
Absorbed by atmosphere16%
Reflected by atmosphere6%
Reflected from earth’s surface4%
Absorbed by clouds3%
Total reflected back to space30%

Outgoing Radiation

ComponentPercentage
Radiated to space from clouds and atmosphere64%
Radiated directly to space from earth6%
Radiation absorbed by atmosphere15%
Carried to clouds by latent heat in water vapour23%
Conduction and rising air7%

IMPORTANT

51% of incoming solar radiation is absorbed by land and oceans. 30% is reflected back to space (albedo). Only a tiny fraction of the absorbed energy is used by plants for photosynthesis.

Agricultural insight: Incoming radiation from the sun is short-wave radiation (visible). Outgoing radiation from the earth’s surface is long-wave radiation (infrared, not visible). Greenhouse gases trap this outgoing long-wave radiation, causing global warming.


Light — The Visible Spectrum

Light is the visible portion of the solar spectrum with wavelength range from 0.39 to 0.76 micron (390–760 nm).

Light lies between UV and IR radiation. Three properties of light matter for crops: intensity, quality (wavelength), and duration (photoperiod).

Effects of Light on Plants

EffectDetailAgricultural Example
PhotosynthesisLight is indispensable for photosynthesisAll crop production depends on it
Plant structureAffects tillers, culm strength, leaf size, root developmentRice tillering increases with adequate light
Poor light effectsCauses plant abnormalities, weak stems, elongated internodesLodging in shaded rice crops

Plants Classified by Light Response

TypeDescriptionExamples
Sciophytes (shade-loving)Grow better under partial shadeBetel vine, buckwheat, ginger, turmeric
Heliophytes (sun-loving)Produce maximum dry matter under high light with adequate moistureMaize, sorghum, rice, sugarcane, cotton

Spectrum of Radiation

Solar radiation spans a wide range of wavelengths, from cosmic rays to infrared:

BandSpectrumWavelength (micron)Effect on Agriculture
UltraCosmic rays< 0.005Lethal; filtered by atmosphere
UltraGamma rays, X-rays0.005–0.20Lethal; filtered by atmosphere
UltraUltraviolet rays0.20–0.39Kills bacteria and fungi; used in seed sterilisation
Visible (PAR)Violet0.39–0.45Strong formative effect on plant tissue
Visible (PAR)Blue0.45–0.49Strong chlorophyll absorption; photosynthesis
Visible (PAR)Green0.49–0.57Low absorption (reflected — why plants look green)
Visible (PAR)Yellow0.57–0.59Low photosynthetic effectiveness
Visible (PAR)Orange0.59–0.62Moderate photosynthetic activity
Visible (PAR)Red0.62–0.75Most favourable for growth; highest photosynthesis
InfraredInfrared rays> 0.75Thermal energy; source of heat for plants

NOTE

Key exam facts: Red light is the most favourable for plant growth, followed by violet-blue. UV kills bacteria and fungi. Infrared provides heat but excess is detrimental.


Wavelength Effects on Plants — Detailed

BandWavelength (nm)Effect on Crops
1> 1000No specific effect; absorbed radiation converts to heat
2720–1000Plant elongation; far-red (700–920 nm) affects photoperiodism, seed germination, flowering, fruit colour
3510–720Strongly absorbed by chlorophyll; maximum photosynthesis and photoperiod response
4510–610Green-yellow; low photosynthetic effectiveness
5400–510Strongest chlorophyll and yellow pigment absorption; strong formative effect on tissue
6315–400Formative effects; thickening of leaf tissue
7280–315Detrimental to most plants
8< 280Lethal — UV germicidal action kills plants

Light Intensity

  • Light intensity is measured by comparing with a standard candle. The oldest unit is Lux.
  • About 1% of light energy is converted into biochemical energy through photosynthesis.

Effects of Extreme Light

ConditionEffectAgricultural Example
Very low lightReduces photosynthesis; weak growthShaded lower leaves in dense maize canopy
Very high lightIncreases respiration; causes solarisation (photo-oxidation) — oxidation of cell contentsLeaf scorching in transplanted seedlings

Critical Light Stages for Crops

CropCritical Period for LightSignificance
MaizeThird month after sowingGrain filling; light shortage reduces yield
Rice25 days prior to floweringPanicle development; cloudy weather reduces grain number
BarleyAt flowering periodPollination and grain set

Photosynthetically Active Radiation (PAR)

PAR ranges between 400–700 nm — the same as visible light — and is the radiation used in photosynthesis.
PropertyDetail
PAR range400–700 nm
Strongest photosynthetic bandsRed and Blue
Highest photosynthesisRed light band
Energy conversionOnly ~1% of PAR is converted to plant biomass

Light Compensation Point

The minimum light intensity at which the rate of respiration equals the rate of photosynthesis. Below this point, the plant consumes more energy than it produces.

PropertyValue
Directly proportional toTemperature
Heliophytes (general)50 ft candle
Rice at 16°C600 ft candle
Rice at 27°C1400 ft candle
C3 vs C4Light compensation point: C3 > C4

Light Saturation Point

The maximum light intensity at which the rate of photosynthesis reaches its maximum. Beyond this, more light does not increase photosynthesis.

Crop TypeLight Saturation (ft candle)
Heliophytes (field crops)~2500
Sciophytes (shade species)~1000

C3 vs C4 Plants — Light Response Comparison

PropertyC3 PlantsC4 Plants
Light compensation pointHigherLower
Light saturation2,500–5,000 ft candle8,000–10,000 ft candle
Photosynthetic rateLowerAbout twice that of C3
ExamplesRice, wheat, barley, soybeanMaize, sorghum, sugarcane, bajra

Light Saturation of Specific Crops

CropLight Saturation (ft candle)C3 or C4
Sugarcane6000C4
Rice5000–6000C3
Wheat5300C3
Sugar beet4400C3
Potato3000C3
Maize2500–3000C4

TIP

Sugarcane and Rice have the highest light saturation values (5000–6000 ft candle). Sugarcane utilizes up to 10–12% of total solar energy — the highest among crops.


Photoperiodism

Photoperiodism is the response of plants to the relative length of day and night (photoperiod), which controls flowering.
CategoryDay Length TriggerExamples
Short-day plantsFlowering when day length < 12 hoursRice, Soybean, Tobacco, Chrysanthemum
Long-day plantsFlowering when day length > 12 hoursBarley, Oat, Radish, Sugarbeet, Carrot, Cabbage
Day-neutral plantsFlowering based on age, not day lengthTomato, Maize, Sunflower
  • Short-day plants are typically tropical crops (near the equator, shorter days during growing season).
  • Long-day plants are typically temperate crops (longer summer days trigger flowering).
  • Day-neutral plants flower after reaching a certain maturity — photoperiod has no effect.

TIP

Exam tip: Rice = short-day, Barley/Oat = long-day, Tomato/Maize = day-neutral. Remember: “Rice Short” (both have ‘r-s’ sounds). Long-day plants are mostly rabi/temperate crops.


Latitude and Climate Zones

Latitude determines the angle of solar radiation, day length, and seasonal patterns — which in turn decide what crops can grow in a region.

ZoneLatitudeCharacteristicsCrop Associations
Tropical0–23.5°Near-vertical sun year-round, very warm, high evaporation, frequent cloudsRice, sugarcane, tropical fruits, spices
Sub-tropical23.5–40°Highest summer radiation; most deserts fall in this zoneWheat, cotton, citrus, groundnut
Temperate40–65.5°Mild temperatures; regular precipitation; day length varies 8–16 hoursWheat, barley, apples, potatoes
Polar> 60°Very low radiation; polar days/nights; sparse vegetationVery limited agriculture

NOTE

India spans tropical to sub-tropical latitudes (8°N to 37°N). This is why India can grow both tropical crops (rice, coconut) in the south and temperate crops (apple, saffron) in the high-altitude north.


Role of Temperature in Crop Production

While light quality and duration determine photosynthesis, temperature controls the rate of all biochemical reactions in plants — from enzyme activity to respiration to grain filling.

Temperature RangeSignificance
0°C – 60°CRange for most higher plants
10°C – 40°CRange for most crop plants
15–40°CGeneral optimal range for crop growth
20°C – 30°CMaximum dry matter production

Daily Temperature Patterns

FactValue
Lowest daily temperatureJust before sunrise (earth has radiated heat all night)
Highest daily temperatureAfter 2 PM (earth absorbs more heat than it radiates until early afternoon)
Absolute zero-273°C (theoretical lowest temperature)
Sea surface temperature (normal)23°C
  • At high temperature + high humidity, pests and diseases increase.
  • High night temperature increases respiration, reducing net dry matter accumulation.

Cardinal Temperatures

Every crop has three critical temperature thresholds called cardinal temperatures:

SeasonCropsMinimum (°C)Optimum (°C)Maximum (°C)
Cool seasonWheat, Barley, Potato, Oats0–525–3030–38
Warm seasonRice, Sorghum, Maize, Sugarcane, Bajra, Groundnut, Red gram, Cowpea15–2030–3845–50

IMPORTANT

Cool season crops have lower minimum (0–5°C) and lower maximum (30–38°C). Warm season crops have higher minimum (15–20°C) and higher maximum (45–50°C). This is why wheat fails in summer and rice fails in cold winters.


Heat Injuries

When temperatures exceed a crop’s maximum cardinal temperature, physical damage begins. Excessive heat causes direct injury to plant tissues through three mechanisms:

Injury TypeDescriptionAgricultural Example
Thermal death pointCell death at 50–60°CSeedlings dying on hot bare soil surface
Sun cladBark injury from high day temperature + low night temperatureBark damage on fruit tree trunks in arid regions
Stem girdleStem scorches at ground level due to hot soilSeedling death in transplanted vegetables on exposed soil

Cold Injuries

Just as excessive heat damages crops, temperatures below the minimum cardinal threshold cause injury. Unlike heat damage, cold injuries involve ice formation, dehydration, and oxygen deprivation. Low temperatures damage crops through four distinct mechanisms:

Injury TypeMechanismExample
Chilling injuryYellowing (chlorotic condition) when tropical crops are exposed to temperatures below 20°CChlorotic bands on sugarcane, sorghum, and maize leaves in winter
Freezing injuryWater freezes as ice crystals in intercellular spaces; protoplasm dehydrates and cells dieFrost damage in potato and tea in north India
SuffocationIce/snow cover prevents oxygen entry and CO₂ exit from rootsWinter crop damage in temperate hill regions
HeavingIce crystals increase soil volume, physically lifting plants from the groundUprooting of young wheat plants in Kashmir

WARNING

Exam-critical thresholds: Thermal death point = 50–60°C. Chilling injury begins below 20°C night temperature in tropical crops. Frost damage is worse on sandy soils (poor heat retention). Remember: average earth surface temperature = 14–15°C.


Oasis Effect

The oasis effect is a local microclimate phenomenon where a vegetated or irrigated area is cooler than its surrounding dry environment.

This occurs because:

  1. Evapotranspiration (ET) from the vegetation uses latent heat, cooling the air above the crop.
  2. Higher albedo of green vegetation reflects more solar radiation compared to bare dry soil.

Example: An irrigated wheat field surrounded by arid desert in Rajasthan will have a noticeably cooler microclimate than the surrounding barren land — this is the oasis effect.

TIP

Exam one-liner: Oasis effect = local cooling due to ET and higher albedo of vegetation surrounded by dry area.


Summary Table

TopicKey FactExam Value
ConvectionPredominant form of energy transfer on earthDefinition question
Solar constant1.94 cal/cm²/min (1 Langley/min)Numerical question
Albedo — highestIce: 90%Comparison question
Albedo — lowestBlack moist soil: 8%Comparison question
Earth’s average albedo30%Numerical question
Energy absorbed by land/oceans51% of incoming solar radiationPercentage question
Light wavelength range0.39–0.76 micron (390–760 nm)Range question
PAR range400–700 nmRange question
Best light for growthRed lightColour question
Light compensation pointC3 > C4Comparison question
Light saturation — C48,000–10,000 ft candleNumerical question
Sugarcane efficiencyUses 10–12% of total solar energyPercentage question
Critical stage — Rice25 days before floweringTiming question
Cardinal temp — cool cropsMin 0–5°C, Max 30–38°CTemperature range
Cardinal temp — warm cropsMin 15–20°C, Max 45–50°CTemperature range
Maximum dry matter production20–30°CTemperature range
Thermal death point50–60°CThreshold question
Chilling injury thresholdBelow 20°C night temperatureThreshold question
Frost damage — worst onSandy soilsSoil type question
Greenhouse concept byJ.B. FourierScientist question
Photoperiodism — short-dayRice, Soybean, Tobacco (< 12 h)Classification question
Photoperiodism — long-dayBarley, Oat, Radish, Sugarbeet (> 12 h)Classification question
Photoperiodism — day-neutralTomato, Maize (age-based)Classification question
Optimal crop growth range15–40°CTemperature range
Lowest daily temperatureJust before sunriseTiming question
Highest daily temperatureAfter 2 PMTiming question
Absolute zero-273°CNumerical question
Sea surface temperature23°CNumerical question
Tropical zone0–23.5° latitudeZone question
Sub-tropical zone23.5–40° latitudeZone question
Temperate zone40–65.5° latitudeZone question
Oasis effectLocal cooling due to ET + higher albedoDefinition question

Summary Cheat Sheet

Concept / TopicKey Details
ConvectionPredominant form of energy transfer on earth
Solar constant1.94 cal/cm²/min (1 Langley/min)
Albedo — highestIce: 90%
Albedo — lowestBlack moist soil: 8%
Earth’s average albedo30%
Energy absorbed by land/oceans51% of incoming solar radiation
Light wavelength range0.39-0.76 micron (390-760 nm)
PAR range400-700 nm (= visible light)
Best light for growthRed light
Light compensation pointC3 > C4
Light saturation — C48,000-10,000 ft candle
Sugarcane solar efficiencyUses 10-12% of total solar energy (highest)
Critical stage — Rice25 days before flowering
Cardinal temp — cool cropsMin 0-5°C, Max 30-38°C
Cardinal temp — warm cropsMin 15-20°C, Max 45-50°C
Maximum dry matter production20-30°C
Thermal death point50-60°C
Chilling injury thresholdBelow 20°C night temperature in tropical crops
Frost damage worst onSandy soils (poor heat retention)
Average earth surface temp14-15°C
Optimal crop growth range15-40°C
Lowest daily tempJust before sunrise
Highest daily tempAfter 2 PM
Absolute zero-273°C
Sea surface temp (normal)23°C
Photoperiodism — short-dayRice, Soybean, Tobacco (< 12 h)
Photoperiodism — long-dayBarley, Oat, Radish, Sugarbeet (> 12 h)
Photoperiodism — day-neutralTomato, Maize (age-based)
Tropical zone0-23.5° latitude
Sub-tropical zone23.5-40° latitude
Temperate zone40-65.5° latitude
Oasis effectLocal cooling from ET + higher albedo of vegetation

TIP

Next: Lesson 05 covers humidity, wind, and evapotranspiration — the three forces that govern crop water balance, pest pressure, and atmospheric moisture movement.

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