Formula Used:
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Net heat exchange between two surfaces represents the amount of heat that is transferred per unit of time through radiation between two bodies. It is typically measured in watts (joules per second) and depends on the radiosity values of both surfaces, their surface areas, and the radiation shape factor between them.
The calculator uses the formula:
Where:
Explanation: The formula calculates the net radiation heat transfer between two surfaces based on their radiosity difference and the geometric configuration represented by the shape factor.
Details: Accurate calculation of radiation heat transfer is crucial for thermal system design, energy efficiency analysis, and understanding heat exchange processes in various engineering applications including HVAC systems, industrial furnaces, and electronic cooling.
Tips: Enter radiosity values in W/m², surface area in m², and radiation shape factor (between 0 and 1). All values must be valid (radiosity ≥ 0, surface area > 0, shape factor between 0-1).
Q1: What is radiosity?
A: Radiosity represents the rate at which radiation energy leaves a unit area of a surface in all directions, including both emitted and reflected radiation.
Q2: What is radiation shape factor?
A: Radiation shape factor (or view factor) is the fraction of radiation energy radiated by one surface that is incident on another surface when both surfaces are placed in a non-absorbing medium.
Q3: What are typical values for radiation shape factor?
A: Shape factor values range from 0 (no radiation exchange) to 1 (complete enclosure). The value depends on the geometric configuration and orientation of the surfaces.
Q4: When is this calculation most applicable?
A: This calculation is most applicable for gray, diffuse surfaces in thermal radiation analysis where the medium between surfaces is non-participating (doesn't absorb, emit, or scatter radiation).
Q5: How does surface area affect heat transfer?
A: Larger surface areas generally result in greater heat transfer rates, as the radiation exchange is proportional to the surface area of the emitting body.