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Fundamentals of Heat Transfer Part 1
Rating: 4.5 out of 5(153 ratings)
5,110 students

Fundamentals of Heat Transfer Part 1

Learn the Fundamentals of Heat Transfer and Thermodynamics: From Conduction to Radiation and Beyond
Created byProf. Samer
Last updated 12/2020
English
English [Auto],

What you'll learn

  • Perform general energy balances as well as surface energy balances
  • Understand the basic mechanisms of heat transfer, which are conduction, convection, and radiation
  • Obtain the differential equation of heat conduction in various coordinate systems, and simplify it for steady one-dimensional case
  • Identify the thermal conditions on surfaces, and express them mathematically as boundary and initial conditions
  • Solve one-dimensional heat conduction problems and obtain the temperature distributions within a medium and the heat flux
  • Understand the concept of thermal resistance and its limitations, and develop thermal resistance networks for practical heat conduction problems
  • Solve steady conduction problems that involve multilayer rectangular, cylindrical, or spherical geometries
  • Develop an intuitive understanding of thermal contact resistance, and circumstances under which it may be significant
  • Identify applications in which insulation may actually increase heat transfer
  • Analyze finned surfaces, and assess how efficiently and effectively fins enhance heat transfer
  • Assess when the spatial variation of temperature is negligible, and temperature varies nearly uniformly with time, making the lumped system analysis applicable

Course content

5 sections46 lectures8h 15m total length
  • What and How?19:05

    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.

  • Conduction17:54

    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.

  • Example 14:08

    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.

  • Convection14:37

    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.

  • Radiation17:10

    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.

  • Example 28:30

    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.

  • Conservation of Energy22:06

    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.

  • Example 35:27

    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.

  • Example 48:15

    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.

  • Surface Energy Balance4:44

    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.

  • Example 57:45

    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.

  • Example 614:01

    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.

Requirements

  • Fundamentals of Fluid Mechanics course.
  • Fundamentals of Engineering Thermodynamics course.

Description

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.

Who this course is for:

  • Engineering Students
  • Engineers curious about heat transfer