Updated Engineering & Physics

Heat Transfer Coefficient Calculator Suite

Analyze heat transfer by conduction, convection, radiation and overall U in one place. Compute k, h, U, thermal resistance and heat flow with support for °C, °F and Kelvin.

Conduction & Thermal Resistance Convection Coefficient (h) Radiation Coefficient (hr) Overall U & Q = U·A·ΔT

Interactive Heat Transfer Coefficient Calculator

Use the tabs to work with conduction through solids, convection between a surface and a fluid, radiation between a surface and surroundings, and overall heat transfer with multiple resistances in series. Choose °C, °F or K for temperature inputs and set decimal precision to match your reporting needs.

Conduction mode assumes one-dimensional steady-state heat transfer through a single, uniform layer. U and R are computed from the layer only (no convection films). Use the Overall U tab to add convection.

Convection mode uses Newton’s law of cooling q = h·(Ts − T). Provide heat flux and the temperature difference between the surface and the fluid.

Radiation mode uses the Stefan–Boltzmann law. An effective radiation coefficient hr is computed so that q = hr·(Ts − Tsur) mimics the non-linear radiative heat flux.

Overall mode models a single solid layer with convection on both sides: U = 1 / (1/h₁ + L/k + 1/h₂). For more layers you can combine multiple L/k terms into an equivalent conduction resistance.

Heat Transfer Coefficient Calculator – Conduction, Convection, Radiation & Overall U

Heat transfer coefficients are central to thermal analysis in building design, mechanical engineering, process equipment, electronics cooling and many other applications. This Heat Transfer Coefficient Calculator collects the most common steady-state formulas in one place and lets you work in Celsius, Fahrenheit or Kelvin.

Instead of manually juggling k, h, U, thermal resistance and Q = U·A·ΔT, you can move through four dedicated modes: conduction, convection, radiation and overall heat transfer. Each tab focuses on a standardationship and reports both intermediate and final values so you can follow the physics behind the numbers.

How the Heat Transfer Calculator Is Organized

The suite is split into four modes that match typical engineering questions:

  • Conduction: Thermal conductivity, thickness, U-value, R-value and heat flow through a solid layer.
  • Convection: Convection coefficient h from measured or assumed heat flux and temperature difference.
  • Radiation: Effective radiation coefficient hr and radiative heat flux between a surface and surroundings.
  • Overall: Combined conduction and convection in series to compute overall U and Q through a wall or surface system.

Mode 1 – Conduction Heat Transfer (k, U, R, Q)

Conduction through a plane wall is often modeled with Fourier’s law in one dimension: q = k·(ΔT / L), where q is heat flux (W/m²), k is thermal conductivity (W/m·K), L is thickness (m) and ΔT is the temperature difference across the wall.

In the conduction tab you enter:

  • Thermal conductivity k (W/m·K)
  • Layer thickness L (m)
  • Area A (m²)
  • Temperatures on the hot and cold sides
  • Your preferred temperature unit (°C, °F or K) and decimal precision

The calculator converts the temperatures to Kelvin internally, computes ΔT, then uses:

  • R = L / k (m²·K/W) – conduction resistance of the layer
  • U = 1 / R (W/m²·K) – conduction heat transfer coefficient
  • Q = U·A·ΔT (W) – total heat transfer rate
  • q = Q / A (W/m²) – corresponding heat flux

Mode 2 – Convection Heat Transfer Coefficient h

Convection between a surface and a fluid is often described using Newton’s law of cooling: q = h·(Ts − T). If you know the heat flux and the surface and fluid temperatures, you can rearrange this to solve for h.

In the convection tab you provide:

  • Heat flux q (W/m²)
  • Surface temperature Ts
  • Fluid (bulk) temperature T
  • Temperature unit (°C, °F or K) and decimal precision

The calculator converts temperatures to Kelvin to compute ΔT and then calculates the convection coefficient: h = q / ΔT. This is useful when estimating h from experimental measurements or when back-calculating h from known fluxes in equipment or building components.

Mode 3 – Radiation Heat Transfer Coefficient hr

Thermal radiation between a surface and its surroundings can be described by the Stefan–Boltzmann law. For a diffuse, gray surface exchanging radiation with a large isothermal surrounding, an effective radiation coefficient hr can be defined so that q ≈ hr·(Ts − Tsur).

In the radiation tab you enter:

  • Surface temperature Ts
  • Surroundings temperature Tsur
  • Emissivity ε between 0 and 1
  • Temperature unit (°C, °F or K) and decimal precision

The tool converts temperatures to Kelvin, applies the Stefan–Boltzmann constant and reports:

  • ΔT in Kelvin
  • Effective radiation coefficient hr (W/m²·K)
  • Radiative heat flux q (W/m²)

Mode 4 – Overall Heat Transfer Coefficient U and Heat Flow

Many practical systems combine conduction through a wall and convection on both sides. The resistances add in series: 1/h₁ on the inside, L/k through the wall and 1/h₂ on the outside. The overall heat transfer coefficient U is then:

U = 1 / (1/h₁ + L/k + 1/h₂)

In the overall mode you specify:

  • Inner convection coefficient h₁ (W/m²·K)
  • Wall conductivity k (W/m·K) and thickness L (m)
  • Outer convection coefficient h₂ (W/m²·K)
  • Area A (m²)
  • Inside and outside temperatures with unit (°C, °F or K)

The calculator sums the resistances, inverts to get U, computes ΔT and then reports Q = U·A·ΔT and the corresponding heat flux. For multi-layer constructions you can extend the method by combining several L/k terms into a total conduction resistance before using this tab.

Tips for Using the Heat Transfer Coefficient Calculator

  • Keep units consistent for area, thickness and conductivity; the calculator assumes SI units (m, m², W/m·K).
  • Use °C, °F or K for temperatures as convenient; the calculator handles the necessary conversions internally.
  • Start with the conduction tab to understand how wall thickness and material affect U.
  • Use the convection and radiation tabs to estimate h and hr when building an overall resistance model.
  • Finish in the overall tab to see the combined effect on U and Q for your system or building element.

The results are idealized steady-state values and do not include transient effects, multidimensional heat flow or complex geometries. Always combine these estimates with engineering judgment and, where needed, applicable codes and standards.

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Heat Transfer Coefficient FAQs

Frequently Asked Questions Heat Transfer Coefficients

Quick answers before you plug numbers into conduction, convection, radiation and overall U calculations.

No. Thermal conductivity k is a material with units W/m·K and applies to conduction through a solid. The overall heat transfer coefficient U, also in W/m²·K, includes conduction plus convection on one or both sides and is defined for the entire surface or construction, not just the material itself.

Yes, in a simplified way. For several layers in series, you can sum the conduction resistances L/k for each layer, add 1/h terms for surface films, and then take the reciprocal of the total resistance to get U. This calculator explicitly supports one layer plus inner and outer convection; you can pre-calculate a combined conduction resistance for multiple layers and enter it by adjusting k and L accordingly.

Many heat transferationships depend on absolute temperature differences and radiation terms that must use Kelvin for consistency. The calculator converts your entries from °C or °F to Kelvin for the physics and then formats the results in your chosen display unit so that you see familiar values and units while the internal math stays correct.

Very small or zero temperature differences can lead to extremely large or undefined coefficients when rearranging formulas (for example, h = q / ΔT). The calculator checks for tiny ΔT values and will warn you or produce very large coefficients that should be interpreted with caution. Physically, negligible ΔT implies negligible driving force for heat flow.

This tool is built for steady-state, one-dimensional equivalent models. Transient problems, fins, complex geometries and multidimensional heat flow often require numerical methods or specialized software. You can still use the results here as a quick reference or as input to more advanced models, but they will not capture time-dependent or 2D effects.