
Explore what heat transfer is and how it occurs, driven by a nonzero temperature difference, with heat moving from hot to cold through conduction, convection, and radiation.
Explore conduction from a microscopic view in gases, liquids, solids, detailing energy transfer by collisions, lattice vibrations, and free electrons; define thermal conductivity, Fourier's law, and copper, water, air.
Compute steady-state heat loss through a 0.15 m brick wall (k=1.7) with 1400 K to 1150 K. The area is 0.6 m^2, yielding about 1.7 kW.
Examine convection on a fixed flat plate, with thermal boundary layers and conduction-to-convection heat transfer governed by Newton's law of cooling. Show how convection coefficient and geometry shape boundary-layer thickness.
Explore how radiation transfers energy without a medium, using black-body emissive power and the Stefan-Boltzmann law, and how absorptivity, reflectivity, and irradiation govern net heat transfer.
Calculate heat loss from an uninsulated 70 mm steam pipe at 200 °C (emissivity 0.8) in 25 °C air using convection and Stefan–Boltzmann radiation per unit length.
Explore the conservation of energy in open systems, detailing the energy balance that links changes in stored energy to heat transfer, work transfer, mass transfer, and energy generation.
Analyze steady-state heat transfer in a rectangular duct by using the ideal gas law to get density and cross-sectional area for mass flow, then compute Q from ΔT and cp.
Derives the transient temperature variation of a long conducting rod by applying the energy balance with electrical energy generation, convection to ambient air, and radiation to the surroundings.
present the surface energy balance for a wall with convection from moving air, radiation from the surroundings, and conduction inside the wall, noting the surface stores no energy.
Apply a steady-state surface energy balance at the outer brick wall, balancing conduction, convection, and radiation. Use Fourier's law to show a linear temperature distribution and solve for wall temperature.
Explores heat transfer from a human body through a 3 mm skin-fat layer (k=0.3) with 35 c temperature and emissivity 0.95, balancing conduction, convection, and radiation for air and water.
Introduce thermal diffusivity alpha as k over rho c_p, the volumetric heat capacity. Larger alpha means faster heat propagation; small alpha implies poor conduction and slow temperature change.
Derive the heat diffusion equation from a differential control volume in Cartesian coordinates, applying Fourier's law and a generation term to model conduction.
Derives the heat diffusion equation in cylindrical coordinates with radial, angular, and axial terms, noting a steady-state, no-generation case where radial temperature varies logarithmically, unlike linear plane walls.
Derive the heat diffusion equation in spherical coordinates via a control volume, apply an energy balance, and show steady-state no-generation conduction yields a 1/r temperature profile.
Explore how boundary and initial conditions define unique solutions to the heat diffusion equation. 1d steady state needs two boundaries; 2d needs six; transient 1d requires an initial condition.
Explore the three main boundary conditions for one-dimensional heat conduction: Dirichlet with fixed surface temperature; constant heat flux (adiabatic case); and convection boundary condition.
Determine the temperature distribution in a 0.2 m thick wall under one-dimensional steady-state heat conduction with no generation, between 120 and 50 c, and compute the 6.3 kw heat flux.
Analyze one-dimensional steady-state heat transfer in a 0.5 cm thick, 300 cm² baseplate with inner heat flux and outer convection to obtain the temperature distribution and surface temperatures.
An example explores radial steady-state conduction in a cylindrical steam pipe, deriving a logarithmic temperature distribution under Dirichlet boundaries T1=150 C and T2=60 C, and calculating heat loss 0.79 MW.
Derive the steady-state temperature distribution in a spherical shell under Dirichlet conditions and calculate the heat loss with k=45, inner T=200 C, outer T=80 C.
Explore the thermal resistance concept for steady-state conduction, convection, and radiation, using an electrical circuit analogy to derive series and parallel resistances in a plane wall.
Analyze a composite wall with layers of different thermal conductivities and thicknesses, examining one-dimensional conduction, temperature distribution, and convection to estimate heat transfer.
Examine thermal contact resistance at interfaces in multilayer solids, where imperfect contact and air gaps cause temperature drops and influence heat flux.
Model heat transfer through a double pane window by combining convection and conduction in series across glass and air, showing the air gap's insulation and comparing to a single pane.
Analyze one-dimensional heat transfer through a multi-layer wall, using parallel conduction through plaster, brick, and foam, with indoor and outdoor convection to calculate heat loss.
Derives radial thermal resistances for a cylinder - inner convection, wall conduction, outer convection - and links overall heat loss to temperature differences with a series resistance model.
Analyze radial heat transfer in a hollow sphere with inner and outer convection. Compute conduction through the sphere wall and the total resistance using 4 pi k and 1/R relationships.
Learn how multilayer cylinders and spheres transfer heat radially by combining conduction resistances in series with inner and outer convection to predict heat loss.
Model heat transfer for a 3 m diameter spherical ice-water tank, including inner convection, wall conduction, outer convection and black-body radiation, and estimate ice melted over 24 hours.
The lecture analyzes heat loss from a steam pipe by combining convection and radiation into a single thermal resistance. It shows insulation increasing resistance and reducing heat loss.
Determine the critical radius of insulation to minimize heat gain by balancing conduction and convection, and select an insulation thickness above this value for maximum overall thermal resistance.
Derive the one-dimensional steady-state heat equation with volumetric energy generation, solving for the temperature distribution in a wall under convection on both sides and using energy balance.
Analyze heat transfer from thin fins attached to a solid, deriving temperature distribution by conduction and convection with base and adiabatic-tip conditions, including corrected length for rectangular and cylindrical fins.
Define fin efficiency as the ratio of actual to maximum heat transfer. Infinite conductivity yields no temperature drop; longer fins reduce efficiency, while corrected length accounts for center heat transfer.
Determine the proper length of a finite-length fin in heat transfer using tangent hyperbolic relations to compare finite and infinitely long fins, balancing heat transfer with size and cost.
Fin effectiveness is the ratio of heat transfer from the fin to the heat transfer from the base without a fin, depending on fin efficiency and the surface-area-to-cross-sectional-area ratio.
Compute the overall effectiveness by comparing heat transfer with fins attached to a surface to the unfinned case, using fin area, fin efficiency, and surface dimensions.
Design aluminium fins to dissipate heat from an integrated circuit board using convection. Compute fin efficiency and overall effectiveness to determine the required number of fins.
Analyze heat transfer from a transistor to an aluminium sleeve, including thermal contact resistance, sleeve conduction, and air convection via fins.
Apply the lumped capacitance method to transient heat conduction with a uniform temperature. Obtain exponential decay with time constant tau = ρ V Cp /(h A) and an RC-like analogy.
Assess the validity of the lumped capacitance method by ensuring negligible temperature gradients and uniform temperature, using the Biot number and conduction–convection resistance across planes, cylinders, and spheres.
We model a spherical thermocouple to determine a 0.706 m diameter for a 1 s time constant, using lumped capacitance to reach 199 °C in about 5.16 s.
Calculate the air velocity to cool plates from 700°c to 50°c in a 10 m cooling chamber at 4 cm/s, using lumped capacitance and a biot number check.
Welcome to our comprehensive course on Heat Transfer and Thermodynamics! In this course, we delve into the fundamental concepts and principles that govern the transfer of heat energy, including conduction, convection, and radiation.
Our objective is to equip you with a solid foundation in the modes of heat transfer and the relations used to calculate heat transfer rates. We begin by answering the crucial questions of What is heat transfer? and How is energy transferred by heat? These questions set the stage for a deep dive into the underlying principles of heat transfer processes.
We explore how the heat equation, which is based on Fourier's law and the conservation of energy requirement, can be used to obtain the temperature distribution within a medium for both steady-state and transient conditions. Furthermore, we demonstrate how thermal circuits can be employed to model steady-state heat flow in common geometries such as plane walls, cylinders, spheres, and extended surfaces (fins).
In addition, we discuss the lumped capacitance method, which is appropriate when a single temperature can be used to characterize the time response of the medium to the boundary change, and we use it to solve transient conduction problems.
By the end of this course, you will have a comprehensive understanding of the modes of heat transfer, the principles that govern them, and how they can be applied to solve problems in thermal systems engineering.
If you are interested in expanding your knowledge of Heat Transfer and Thermodynamics, this course is perfect for you. Join us today and take the first step towards becoming an expert in the field.