What is Heat Transfer?

Heat transfer is a discipline of thermal engineering that concerns the generation, use, conversion, and exchange of thermal energy between physical systems. Heat transfer is classified into various mechanisms, such as thermal conduction, thermal convection, thermal radiation, and transfer of energy by phase changes

In general, heat transfer describes the flow of heat (thermal energy) due to temperature differences and the subsequent temperature distribution and changes.

Heat Transfer

According to thermodynamic systems, heat transfer is defined as

The motion of heat across the border of the system due to a difference in temperature among the device and its surroundings. Interestingly, the difference in temperature is said to be a ‘potential’ that causes the transfer of heat from one point to another. Besides, heat is also known as flux.

Heat Transfer Methods

Heat can travel shift from one place to another in several ways. The different modes of heat transfer include:

• Conduction
• Convection

Meanwhile, if the temperature difference exists between the two systems, heat will find a way to transfer from the higher to the lower system.

Conduction of Heat Transfer

The process in which heat flows from objects with higher temperature to objects with lower temperature.

An area of higher kinetic energy transfers thermal energy towards the decrease kinetic energy area. High-speed particles clash with particles transferring at a slow speed, as a result, slow speed particles increase their kinetic energy. This is a typical form of heat transfer and takes location through physical contact. Conduction is also known as thermal conduction or heat conduction.

Conduction Equation

The coefficient of thermal conductivity shows that a metal body conducts heat better when it comes to conduction. The rate of conduction can be calculated by the following equation:

Q = [K.A.(ThotTcold)]d

Where,

• Q is the transfer of heat per unit time
• K is the thermal conductivity of the body
• A is the area of heat transfer
• Thot is the temperature of the hot region
• Tcold is the temperature of the cold region
• d is the thickness of the body

Conduction Examples

Following are the examples of conduction:

• Ironing of clothes is an example of conduction wherein the heat is conducted from the iron to the clothes.
• Heat is transferred from hands to ice cube resulting in the melting of an ice dice while held in hands.
• Heat conduction through the sand on the beaches. This can be experienced during summers. Sand is a good conductor of heat.

Convection of Heat Transfer

The movement of fluid molecules from higher temperature regions to lower temperature regions.

Convection Equation

As the temperature of the liquid increases, the liquid’s volume also has to increase by the same factor and this effect is known as displacement. The equation to calculate the rate of convection is as follows:

Q = hc ∙ A ∙ (Ts – Tf)

Where,

• Q is the heat transferred per unit time
• Hc is the coefficient of convective heat transfer
• A is the area of heat transfer
• Ts is the surface temperature
• Tf is the fluid temperature

Convection Examples

Examples of convection include:

• Boiling of water, that is molecules that are denser move at the bottom while the molecules which are less dense move upwards resulting in the circular motion of the molecules so that water gets heated.
• Warm water around the equator moves towards the poles while cooler water at the poles moves towards the equator.
• Blood circulation in warm-blooded animals takes place with the help of convection, thereby regulating the body temperature.

Thermal radiation is generated by the emission of electromagnetic waves. These waves carry away the energy from the emitting body. Radiation takes place via a vacuum or transparent medium which can be either solid or liquid. Thermal radiation is the result of the random movement of molecules in the matter. The motion of charged electrons and protons is responsible for the emission of electromagnetic radiation.

As temperature rises, the wavelengths in the spectra of the radiation emitted decreases and shorter wavelengths radiations are emitted. Thermal radiation can be calculated by Stefan-Boltzmann law:

P = e ∙ σ ∙ A· (Tr – Tc)4

Where,

• P is the net power of radiation
• A is the area of radiation
• Tr is the radiator temperature
• Tc is the surrounding temperature
• e is emissivity and σ is Stefan’s constant