Solar Radiation

1Where is the building?

Pick the weather station nearest your site. Skip it and London Heathrow is used.

Try:

Then drop your model, or open a sample below

kWh/m² on every surface for a year, a season or a single day, with your neighbours casting the shade.

Rhino .3dm.obj / .fbxIFCNever uploaded — opened in your browser

No model to hand? Open a sample

  1. 1Pick the location
  2. 2Load a model or a sample
  3. 3Run and read the facades
About Solar Radiation·Cumulative kWh/m² on every surface across the year.

What Solar Radiation does

Calculates how much solar energy each surface of your model receives over any time period. Output is a colour-coded heatmap useful for shading design, PV placement, and overheating risk.

Input:
.3dm / .obj / .ifc + .epw
Output:
Heat map + facade breakdown
Unit:
kWh/m²

How it works

Every hour of the EPW's direct and diffuse sun is projected onto each surface, with your own geometry casting the shade. Checked against Radiance.

  • Hourly direct and diffuse irradiance from the EPW: no synthetic sky.
  • Neighbours, ground and the building itself cast real shadows; nothing is a form factor.
  • Runs in your browser; a city-scale mode is there for large models.

How to use it

  1. Load a model. A .3dm, .obj, .fbx or .ifc with your design and its neighbours, or open a sample. Layers named Context, Site or Ground cast shade and are not measured.
  2. Pick the weather. The EPW supplies every hour of direct and diffuse sun; without one there is nothing to measure.
  3. Choose what to measure. By default the whole model is measured, and layers named Context, Site or Ground only cast shade. Use Manage Layers to measure specific surfaces; the choice is remembered for that file.
  4. Pick a period. Annual, summer, winter, custom range, or a single day.
  5. Set the grid. The tool picks a cell size from the model and tells you the cell count and rough time before you run. Finer is sharper and slower.
  6. Run and read the results. The rail on the right says which facades are hot, what the roof carries and what to try; click an orientation or layer to see those cells alone.

Best used for

  • Finding which surfaces are worth putting PV on before sizing a system.
  • Ranking shading-device options by how much summer gain they actually remove.
  • Spotting overheating-prone glazing early in the design.
  • Comparing massing options by annual gain on the same facade.

Not a substitute for

  • Energy-model inputs for a compliance submission.
  • Predicting a specific year's generation — the EPW is a typical year.
  • Anything requiring a bankable yield assessment.

Known limits

  • Only geometry you load casts shadows: leave out the neighbours and every number reads high.
  • Ground and surrounding surfaces are treated as diffuse reflectors at a fixed albedo — a glazed tower opposite will reflect more than this models.
  • No spectral or angular glazing behaviour; this is incident radiation on a surface, not transmitted energy.
  • Snow, soiling and seasonal vegetation are not modelled.
  • Result resolution follows the mesh: a coarse model gives coarse shadows.

Read the full Solar Radiation guide →