Kilocalorie (IT) per Hour per Square Foot [kcal(IT)/(h·ft²)]

The unit kilocalorie (IT) per hour per square foot, written as kcal(IT)/(h·ft²), measures heat flux density or thermal power per unit area using the International Table kilocalorie (1 kcal(IT) = 4186.8 J). It represents the amount of heat energy transferred through 1 square foot of surface in 1 hour.

This unit is commonly used in U.S.-based building construction, insulation, and HVAC studies to quantify energy transfer through walls, floors, or roofs. Typical applications include:

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  Heat loss or gain through building materials

  
  
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  Solar energy incident on rooftops or horizontal surfaces

  
  
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  Design and analysis of heating and cooling systems

  
  

Mathematically, heat flux is expressed as:

where q is heat flux in kcal(IT)/(h·ft²), Q is total heat in kilocalories, A is area in ft², and t is time in hours.

Conversion to SI units:

While modern practice uses W/m², kcal(IT)/(h·ft²) remains prevalent in legacy U.S. building and insulation data, offering a convenient way to evaluate thermal energy transfer over a typical hourly timescale.

Watt per Square Meter [W/m²]

The unit watt per square meter (W/m²) measures heat flux density or radiant flux, representing the amount of energy transferred per unit area per unit time. One watt equals 1 joule per second, so 1 W/m² corresponds to 1 joule of energy passing through 1 square meter every second.

This unit is widely used in physics, engineering, meteorology, and solar energy studies to quantify energy transfer rates across surfaces. Examples of applications include:

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  Solar radiation: measuring sunlight incident on a surface

  
  
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  Heat transfer: quantifying conduction or convection per unit area

  
  
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  Building energy analysis: evaluating heat gain or loss through walls and roofs

  
  

Mathematically, the heat flux is expressed as:

where q is heat flux in W/m², Q is energy in joules, A is area in square meters, and t is time in seconds.

For example, solar constant at Earth’s surface is approximately 1361 W/m², indicating the power received per square meter from the Sun outside Earth’s atmosphere.

W/m² is the standard SI unit for energy flux density, replacing older units like cal/cm²·s or Btu/ft²·h, and is essential for thermal engineering, climatology, and renewable energy calculations.