DHI (Diffuse Horizontal Irradiance) is the solar radiation reaching a horizontal surface after scattering by the atmosphere, clouds and aerosols, excluding the direct beam. It is measured in W/m² with a shaded pyranometer, classified under ISO 9060:2018. Solar designers combine DHI with DNI to derive GHI and model transposed irradiance.
DHI vs. GHI and DNI
DHI is one half of the equation that produces GHI:
GHI = DNI × cos(solar zenith angle) + DHI
DNI is the direct beam measured perpendicular to the sun; DHI is everything scattered by clouds, haze, and the atmosphere before it reaches a horizontal surface. A pyranometer with a shading device isolates DHI directly, while an unshaded pyranometer records GHI, subtracting the projected DNI component from GHI gives DHI (or vice versa, depending on which two of the three are measured on site).
Why the Diffuse Component Matters in Design
A site’s DHI fraction is a proxy for how “diffuse” its sky is. Overcast, humid, or hazy locations see a larger share of their annual irradiance arrive as DHI, while clear desert skies are dominated by the direct beam. That split has design consequences:
- Fixed-tilt and tracker yield modeling in PVsyst and similar tools consumes hourly DHI, DNI, and GHI series together, a design built only on GHI totals can misjudge the tracker gain or transposition factor if the underlying DHI/DNI split isn’t representative of the site.
- Bifacial gain depends on diffuse and albedo-reflected light reaching the rear of the module, so DHI (alongside albedo) is a meaningful input wherever bifacial modules are being specified.
- Cloudy-climate sites generally lean more on accurate DHI data, since a larger share of deliverable energy is diffuse rather than direct.
Worked Example
If a horizontal pyranometer records a GHI of 600 W/m² at a given moment, and a shaded (diffuse-only) pyranometer at the same time and location reads a DHI of 100 W/m², then the projected direct-beam component on the horizontal plane is 600 − 100 = 500 W/m². Dividing that by the cosine of the solar zenith angle at that moment recovers the DNI value perpendicular to the sun’s rays, illustrating how the three quantities are always internally consistent.
Data Sources
Meteonorm, NREL’s NSRDB, and Solargis all publish hourly DHI series alongside GHI and DNI, which is the standard input format expected by PVsyst and other yield simulation tools.
Key Takeaways
- DHI = diffuse irradiance on horizontal surface.
- GHI = DNI projected + DHI.
- Higher DHI fraction in cloudy climates.
- Standard hourly data source for PVsyst.
- Critical for cloudy-climate solar yield modeling.
Related Reading
Because DHI only ever shows up as part of an hourly weather file, it’s best understood alongside how that data actually drives a yield study, see how PVsyst tracker yield studies sequence DHI, DNI, and GHI inputs, and how solar simulation software compares in handling irradiance data quality.
Since the diffuse component becomes decisive at lower irradiance angles, it also feeds into P50/P90/P99 yield report confidence levels that lenders scrutinize. For state-wise solar resource data covering the DHI/DNI/GHI split across India, Qbits Energy’s irradiance data guide is a useful reference point.
Disclosure: Qbits Energy is a Heaven Designs group company.
Frequently Asked Questions
4 commonly searched questions about DHI (Diffuse Horizontal Irradiance).
How are DHI, DNI and GHI related?
How is DHI measured?
Why does DHI matter in PV simulation?
What is the difference between DHI and diffuse irradiance?
Need engineering-backed solar designs?
Heaven Designs prepares solar drawings, structural calculations, electrical engineering documents, and project-specific permit plan sets.
Nirav Dhanani