Radiation
Radiative exchange: Q = Gr·σ·(T_a⁴ − T_b⁴).
- thermal
- Modelica Standard Library
- 2 ports
- 1 parameter
radiationLibraryThermalDescription
Radiative heat exchange between two surfaces, following the Stefan–Boltzmann law. The heat flow grows with the difference of the fourth powers of the absolute temperatures.
Example
Cooling a hot part A 10 W part cools through a thermal resistance into a heatsink that convects and radiates to 20 °C.
Also in this example:ConstantStepHeat capacitorThermal conductorThermal resistorConvectionFixed temperatureTemperature sourceFixed heat flowHeat flow sourceTemperature sensorHeat flow sensorTemperature difference sensor
Ports
Conserving terminals 2
-
a
port_aHeat port of surface a. Heat flow Q from a to b enters here.
-
b
port_bHeat port of surface b. Q leaves here.
Parameters
-
Net radiation conductance
Gr0.01 m²≥ 0
Net radiation conductance, in m²: an area weighted by emissivities and view factor. For a small body in large surroundings, Gr = ε · A.
Equations
Q = Gr · σ · (port_a.T⁴ − port_b.T⁴), σ = 5.67 × 10⁻⁸ W/(m²·K⁴) port_a.Q_flow = Q, port_b.Q_flow = −Q
Implementation
Modelica.Thermal.HeatTransfer.Components.BodyRadiationAssumptions and limitations
- Gray, diffuse surfaces with a fixed Gr. No heat storage.
Tips
- Temperatures are absolute; the ports must be in kelvin, as all thermal ports are.
See also
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