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Solar Radiation, Irradiance, and Energy Sum

What solar radiation is

Solar radiation is the total electromagnetic energy emitted by the sun and received at the Earth’s surface.

It includes: - Photosynthetically active radiation (PAR) - Infrared radiation (heat) - Small amounts of ultraviolet radiation

Plants respond to both the quantity and timing of this energy.


Irradiance (W/m²)

Irradiance describes the instantaneous power of incoming solar radiation.

  • Units: watts per square metre (W/m²)
  • Represents energy per second
  • Changes continuously with cloud cover, sun angle, and time of day

High irradiance means high short-term energy input.


Radiant energy / Radiation sum

Radiation sum describes the total accumulated solar energy over time.

Common units: - MJ/m² per day - kWh/m² per day

Radiation sum integrates irradiance over time: - High irradiance for a short time - Moderate irradiance for a long time
Both can produce the same radiation sum.


Why radiation sum matters

Radiation sum is closely linked to: - Biomass accumulation - Yield potential - Sugar production - Crop development rate

Plants respond more strongly to total received energy than to brief peaks.


Relationship to PAR and DLI

  • Only a fraction of solar radiation is PAR
  • PAR is measured as photon flux
  • Daily Light Integral (DLI) converts PAR into a daily total

Solar radiation → PAR → photosynthesis → carbohydrates


Agronomic implications

  • Cloudy days reduce radiation sum even if day length is long
  • High radiation with water stress increases heat load
  • Radiation sum helps explain seasonal yield differences
  • Protected cropping often targets radiation sum, not peak light

Key concept

Growth responds to energy accumulated over time, not just brightness at noon.

Solar Radiation, Irradiance, and Energy Sum

What solar radiation is

Solar radiation is the total electromagnetic energy emitted by the sun and received at the Earth’s surface.

It includes: - Photosynthetically active radiation (PAR) - Infrared radiation (heat) - Small amounts of ultraviolet radiation

Plants respond not just to how bright it is at any moment, but to how much energy they receive over time.


Irradiance (W/m²)

Irradiance describes the instantaneous power of incoming solar radiation.

  • Units: watts per square metre (W/m²)
  • Represents energy received per second
  • Changes continuously with sun angle, cloud cover, shading, and time of day

High irradiance means a strong energy input at that moment, but does not describe total daily energy.

Practical meaning:
“How strong is the sun right now?”


Radiant Energy and Radiation Sum

Radiation sum describes the total accumulated solar energy over a defined period, usually a day.

Common units: - MJ/m² per day - kWh/m² per day

Radiation sum integrates irradiance over time. For example: - Short periods of very high irradiance
- Long periods of moderate irradiance

Both can produce the same radiation sum.

Practical meaning:
“How much solar energy did we receive today?”


Why Radiation Sum Matters to Plants

Plant growth correlates much more closely with total received energy than with brief peaks in brightness.

Radiation sum strongly influences: - Photosynthesis over the day - Carbohydrate production - Biomass accumulation - Yield potential

Short spikes of strong sunlight cannot compensate for low total daily energy.


Relationship to PAR and DLI

Only a portion of solar radiation is usable by plants.

  • PAR (400–700 nm) is the biologically active fraction
  • PAR is measured as photon flux (µmol m⁻² s⁻¹)
  • Daily Light Integral (DLI) converts PAR into a daily total (mol m⁻² day⁻¹)

The chain is: Solar radiation → PAR → photosynthesis → carbohydrates

Radiation sum describes energy availability, while DLI describes biologically usable light.


🧠 Quick Terminology Cheat-Sheet

  • W/m² (Irradiance)
    “How strong is the sun right now?”

  • MJ/m²/day (Radiation sum)
    “How much solar energy did we receive today?”

  • PAR (µmol m⁻² s⁻¹)
    “How much of that energy can plants use right now?”

  • DLI (mol m⁻² day⁻¹)
    “How much usable light did plants get today?”

Plants respond more reliably to daily totals than to instantaneous values.


Linking Radiation Sum to Thermal Time (GDH / GDD)

Plant growth depends on both energy supply and temperature-driven metabolism.

  • Radiation sum provides the energy for photosynthesis
  • Thermal time (GDH/GDD) controls the speed of biochemical processes

Growth is most efficient when: - Radiation is high - Temperature is within the crop’s optimal range

High temperature without sufficient radiation increases respiration losses.
High radiation with extreme temperatures reduces efficiency.

Radiation determines how much growth is possible.
Thermal time determines how fast development progresses.


Why Cool, Bright Days Outperform Hot, Dull Days

This explains many real-world yield and growth patterns.

Cool, bright day

  • High radiation sum
  • Moderate temperatures
  • High photosynthesis
  • Controlled respiration
  • Net carbohydrate gain

Hot, dull day

  • Low radiation sum
  • High respiration demand
  • Reduced photosynthesis
  • Net carbohydrate loss

As a result: - Bright, cool conditions build sugars and yield - Warm, overcast conditions increase stress and reduce performance

This is why: - Crops can stall during cloudy heat - Bright northern summers can outperform expectations - Yield drops often follow warm, dull periods


Greenhouse Radiation Transmission Losses

In protected cropping, not all solar radiation reaches the crop.

Common transmission losses include: - Glass or plastic coverings (10–30%) - Condensation on surfaces - Structural shading (frames, gutters) - Dirt, algae, and dust accumulation - Ageing or degraded plastics

These losses are cumulative and often increase over time.

Key point:
External radiation measurements do not represent the energy available to plants inside the structure.


Agronomic Summary

  • Radiation sum explains seasonal yield variation
  • PAR and DLI describe plant-usable light
  • Thermal time explains development rate
  • Cool, bright conditions maximise efficiency
  • Greenhouse transmission losses must be considered

Plants grow on accumulated energy, not momentary brightness.