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What is heat transfer and what causes it?
What is heat transfer and what causes it?
Heat transfer is thermal energy in transit due to a temperature difference.
Differentiate between thermal energy, temperature, and heat transfer.
Differentiate between thermal energy, temperature, and heat transfer.
Thermal energy is the energy associated with the microscopic behavior of matter, temperature is an indirect measure of that energy, and heat transfer is the transport of thermal energy due to temperature differences.
What is the formula for heat transferred over a time interval?
What is the formula for heat transferred over a time interval?
The heat transferred is denoted by $Q$ and measured in joules (J).
What is conduction in the context of heat transfer?
What is conduction in the context of heat transfer?
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How does knowledge of heat transfer apply to the first law of thermodynamics?
How does knowledge of heat transfer apply to the first law of thermodynamics?
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What is the primary mechanism of heat transfer in conduction?
What is the primary mechanism of heat transfer in conduction?
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How does convection differ from conduction in terms of heat transfer?
How does convection differ from conduction in terms of heat transfer?
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What role does a vacuum play in the transfer of radiant energy?
What role does a vacuum play in the transfer of radiant energy?
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Using Fourier’s Law, how is the heat flux (q'') expressed in one-dimensional conduction?
Using Fourier’s Law, how is the heat flux (q'') expressed in one-dimensional conduction?
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Calculate the heat rate (q) through a wall with specified dimensions and temperatures: if a 0.15 m thick wall has temperatures of 1400 K and 1150 K, and dimensions 0.5 m x 1.2 m, given k = 1.7 W/m.K.
Calculate the heat rate (q) through a wall with specified dimensions and temperatures: if a 0.15 m thick wall has temperatures of 1400 K and 1150 K, and dimensions 0.5 m x 1.2 m, given k = 1.7 W/m.K.
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What does Newton’s law of cooling quantify in terms of convection?
What does Newton’s law of cooling quantify in terms of convection?
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What does the emissive power $E$ represent in radiation heat transfer?
What does the emissive power $E$ represent in radiation heat transfer?
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In the context of radiation, what condition is presented when $ ext{α} = ext{ε}$?
In the context of radiation, what condition is presented when $ ext{α} = ext{ε}$?
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How can the net radiation heat flux between a surface and its surroundings be expressed mathematically?
How can the net radiation heat flux between a surface and its surroundings be expressed mathematically?
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What is the formula for the combined heat transfer from convection and radiation?
What is the formula for the combined heat transfer from convection and radiation?
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Study Notes
What is Heat Transfer?
- Heat transfer is thermal energy in transit due to a temperature difference
- Thermal energy is associated with the motion of atoms and molecules within matter
- This motion includes translation, rotation, vibration, and electronic states
- Thermal energy is directly linked to the temperature of matter
Key Definitions
- Thermal energy: Energy associated with microscopic behavior of matter (Symbol: U or u, Units: J or J/kg)
- Temperature: Indirect assessment of thermal energy stored in matter (Symbol: T, Units: K or °C)
- Heat Transfer: Thermal energy transport due to temperature gradients (Symbol: Q, Units: J)
- Heat: Amount of thermal energy transferred over a specific time interval (Symbol: Q, Units: J)
- Heat Rate: Thermal energy transfer per unit time (Symbol: q, Units: W)
- Heat Flux: Thermal energy transfer per unit time and surface area (Symbol: q", Units: W/m2)
Modes of Heat Transfer
- Conduction: Heat transfer through a solid or stationary fluid due to the random motion of atoms, molecules, and electrons
- Convection: Heat transfer due to the combined influence of bulk and random motion of fluids
- Radiation: Energy emitted by matter as electromagnetic waves due to changes in electron configurations
- Conduction and convection require the presence of temperature variations in a material medium
- Radiation does not require a material medium and is most efficient in a vacuum
Conduction Heat Transfer Rates
- General form of Fourier's Law: q" = -k∇T (where q" is heat flux, k is thermal conductivity, and ∇T is the temperature gradient)
- One-dimensional, steady conduction across a plane wall of constant thermal conductivity: qx = -k * A *(T1 - T2)/L (where qx is the heat rate, A is the area, L is the thickness, and T1 and T2 are the temperatures on either side of the wall)
Convection Heat Transfer Rates
- Newton's Law of Cooling: q" = h (Ts - T∞) (where h is the convection heat transfer coefficient, Ts is the surface temperature, and T∞ is the fluid temperature)
Radiation Heat Transfer Rates
- Emissive power: E = * σ * Ts4 (where E is the emissive power, is the surface emissivity, σ is the Stefan-Boltzmann constant, and Ts is the surface temperature)
- Energy absorption due to irradiation: Gabs = α * G (where α is the surface absorptivity and G is the irradiation)
- Net radiation heat flux from a gray surface: q"rad = σ * (Ts4 - Tsur4) (where ε is the emissivity, σ is the Stefan-Boltzmann constant, and Tsur is the surrounding temperature)
- Radiation heat transfer coefficient: hr = εσ (Ts + Tsur)(Ts2 + Tsur2)
- Combined convection and radiation heat flux: q" = h(Ts - T∞) + hr(Ts - Tsur)
First Law of Thermodynamics in Heat Transfer Analysis
- The First Law of Thermodynamics provides a basis for determining the temperature of a system
- The First Law can be applied to a control volume at an instant: Ein - Eout + Eg = Est
- The First Law can be applied to a control volume over a time interval: Ein - Eout + Eg = ΔEst
Methodology of First Law Analysis
- Define the control surface by a dashed line
- Choose an appropriate time basis
- Identify relevant energy transport, generation, and storage terms
- Write the governing form of the Conservation of Energy requirement
- Substitute appropriate expressions for energy terms
- Solve for the unknown quantity
Summary of Heat Transfer Processes
- Conduction: Diffusion of energy due to random molecular motion (q" = -k∇T)
- Convection: Diffusion of energy due to random molecular motion and fluid motion (q" = h(Ts - T∞))
- Radiation: Energy transfer by electromagnetic waves (q = hr A (Ts - Tsur) or q"rad = εσ (Ts4 - Tsur4))
Typical values of heat transfer coefficients
- Free or Natural Convection: Gases (2-25 W/m2.K), Liquids (50-1000 W/m2.K)
- Forced Convection: Gases (25-250 W/m2.K), Liquids (100-20,000 W/m2.K)
- Convection with Phase Change: 2500-100,000 W/m2.K
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Description
Explore the fundamentals of heat transfer, including key definitions and modes such as conduction, convection, and radiation. This quiz covers the relationship between thermal energy, temperature, and heat transfer mechanisms. Test your understanding of these crucial concepts in thermodynamics.