Solar Chimney

2D companion of the 3D solar chimney: sunlight heats air under glass, the warm air rises up the stack and a turbine harvests the draught.

Switch to 3D

Presets

Playback

Apparatus

Model checks

The science

What is modelled

The collector is a large glazed roof over the ground; the air under it warms and flows inward. The warm air in the tall stack is lighter than the outside air, so the pressure difference at the base drives a flow. A turbine takes a share of that pressure and the rest drives the air through the stack.

Equations

  • Collector heat balance m cp ΔT = A (τα G − U ΔT / 2).
  • Buoyancy pressure ΔP = ρ g H ΔT / T0.
  • Stack flow (1 − x) ΔP = (1 + K) ρ v² / 2, m = ρ As v.
  • Electric power P = ηt x ΔP As v.

Checks run in the page

  • Bisection solution against a separate fixed-point iteration.
  • Energy balance of the collector.
  • Optimum turbine share 2/3 at fixed temperature rise.
  • Order-of-magnitude comparison with a 50 kW prototype.

Honest simplifications

Constant absorptance and loss coefficient, no ground heat storage, no wind, no day cycle and a lumped friction coefficient. Results indicate trends, not a plant design.

What to try
  • Press Short stack and see how strongly the chimney height matters.
  • Move the turbine share and compare the coupled curve with the dashed 2/3 optimum.
  • Press Cloudy morning: output drops far faster than the sunlight.
Power against turbine share
Power against irradiance
Power against chimney height
Air temperature rise along the collector
Made with 🤖 ChatGPT