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ASRAE Student Branch meeting Speaker: Kenneth Simpson USGBC – LEED rating system. Today at 5 pm ECJ 5.410. Lecture Objectives:. Review - Heat transfer Convection Conduction Radiation. Simplified Equation for Forced convection. General equation.
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ASRAE Student Branch meeting Speaker: Kenneth Simpson USGBC – LEED rating system Today at 5 pm ECJ 5.410
Lecture Objectives: • Review - Heat transfer • Convection • Conduction • Radiation
Simplified Equation for Forced convection General equation For laminar flow: For turbulent flow: For air: Pr ≈ 0.7, n = viscosity is constant, k = conductivity is constant Simplified equation: Or:
GOVERNING EQUATIONSNatural convection Continuity • Momentum which includes gravitational force • Energy u, v – velocities , n – air viscosity , g – gravitation, b≈1/T - volumetric thermal expansion T –temperature, – air temperature out of boundary layer, a –temperature conductivity
Characteristic Number for Natural Convection Non-dimensionless governing equations Using L = characteristic length and U0 = arbitrary reference velocity Tw- wall temperature The momentum equation become Gr Multiplying by Re2 number Re=UL/n
Grashof number Characteristic Number for Natural Convection Buoyancy forces Viscous forces The Grashof number has a similar significance for natural convection as the Reynolds number has for forced convection, i.e. it represents a ratio of buoyancy to viscous forces. General equation
Natural convectionsimplified equations For laminar flow: For turbulent flow: For air: Pr ≈ 0.7, n = constant, k= constant, b= constant, g=constant Simplified equation: Even more simple Or: T∞ - air temperature outside of boundary layer, Ts - surface temperature
Forced and/or natural convection In general, Nu = f(Re, Pr, Gr) natural and forced convection forced convection natural convection
Example of general forced and natural convection Equation for convection at cooled ceiling surfaces n
Conductive heat transfer k - conductivity of material • Steady-state • Unsteady-state • Boundary conditions • Dirichlet Tsurface = Tknown • Neumann TS1 TS2 L h Tair
What will be the daily temperature distribution profile on internal surface for styrofoam wall? A. B. External temperature profile T time
What will be the daily temperature distribution profile on internal surface for tin glass? A. B. External temperature profile T time
Short-wave & long-wave radiation • Short-wave – solar radiation • <3mm • Glass is transparent • Does not depend on surface temperature • Long-wave – surface or temperature radiation • >3mm • Glass is not transparent • Depends on surface temperature
Radiation emission The total energy emitted by a body, regardless of the wavelengths, is given by: Temperature always in K ! - absolute temperatures • – emissivity of surface • – Stefan-Boltzmann constant A - area
Surface properties • Emission ( e ) is same as Absorption ( a ) for gray surfaces • Gray surface: properties do not depend on wavelength • Black surface: e = a = 1 • Diffuse surface: emits and reflects in each directionequally absorbed (α), transmitted (τ), and reflected (ρ) radiation
View (shape) factors http://www.me.utexas.edu/~howell/ For closed envelope – such as room
Example: View factor relations F11=0, F12=1/2 F22=0, F12=F21 F31=1/3, F13=1/3 A2 A3 A1=A2=A3 A1
Radiative heat flux between two surfaces Simplified equation for non-closed envelope Exact equations for closed envelope ψi,j - Radiative heat exchange factor
Summary • Convection • Boundary layer • Laminar transient and turbulent flow • Large number of equation for h for specific airflows • Conduction • Unsteady-state heat transfer • Partial difference equation + boundary conditions • Numerical methods for solving • Radiation • Short-wave and long-wave • View factors • Simplified equation for external surfaces • System of equation for internal surfaces