Heat Transport Temperature of a wolf pup.

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Presentation transcript:

Heat Transport Temperature of a wolf pup

Goblet filled with coffee and ice water Thermal plume, Lake Michigan Solar radiation Schlieren image of natural convection. Note laminar-turbulent transition Radiating steel bar Temperature distribution Multiphase flow http://www.geog.ucsb.edu/~jeff/115a/remote_sensing/thermal/thermalirinfo.html

Concepts Storage Source Flux

Heat Storage Internal Energy [E/M]; [J/kg] Temperature Latent heat of vaporization Internal Energy [E/M]; [J/kg] Sensible heat Latent heat of fusion solid liquid vapor Temperature

Heat Storage as Sensible Heat Internal Energy (J/kg) cp=specific heat capacity = Energy/(Mass Temp) Change of sensible heat On a per volume basis Cpr=Energy/(Vol Temp) Sensible heat Temperature

Specific Heat Capacity kJ/(kg K) Water: 4.18 Ice: 2.11 Air: 1.00 CO2: 0.84 Gold: 0.13 Hydrogen: 14 (max) Span factor of 100 Water in upper 90%

Heat Storage as Latent Heat Internal Energy (J/kg) Temperature solid liquid vapor Water Melting water: 334 kJ/kg Heating, 0-100oC: 420 kJ/kg Vaporing water: 2260 kJ/kg

Heat Sources Heat generated internally Friction: fluids, solids, energy dissipation Chemical reaction: Exo, Endothermic Radioactive: Fission, fusion Biological: Metabolism Dielectric: Microwaves, oven Joule: Electrical resistance, toaster

Types of heat transfer Thermal flux Conduction: Static media, Diffusion Convection: Fluid moving, advection Forced; Free or Natural Radiation: Emit and adsorb EM, no media Thermal flux

Radiation T1 T2 Heat transfer flux by radiation “Black” body absorbs all incoming radiation and is a perfect emitter. s = Stefan-Boltzman constant 5.67x10-8 W/(m2 K4) = emissivity (0-1); ~1: black; ~0: shiny T1 T2 Stefan’s Law http://www.thermoworks.com/emissivity_table.html

Thermal Conduction Fourier’s Law, energy flux Thermal conductivity

Thermal conductivity W/(moC) Vacuum: 0.001 Air: 0.02 Water: 0.6 Ice: 2 Steel: 10 Copper: 400 Diamond: 1000 http://web.mit.edu/lienhard/www/ahttv202.pdf

Convection Energy flux: Forced: Fluid flow driven by processes other than thermal, pump etc. Free or Natural: Fluid flow by thermally induced density differences

Convection Energy flux: Forced: Fluid flow driven by processes other than thermal, pump etc. Free or Natural: Fluid flow by thermally induced density differences

Convective heat transfer —fluidsolid Tf Ts b

Convective Heat Transfer Coefficient http://web.mit.edu/lienhard/www/ahttv202.pdf

https://docs. google. com/viewer. url=http%3A%2F%2Fwww. bakker https://docs.google.com/viewer?url=http%3A%2F%2Fwww.bakker.org%2Fdartmouth06%2Fengs150%2F13-heat.pdf

Conservation of Heat Energy Governing Equation Conservation of Heat Energy c =cprnT Storage Advective Flux Diffusive Flux (Fick’s Law) Dispersive Flux Source Governing S = Sh

Simulation of Heat Transport

Parameters cp heat capacity r density Kh thermal conductivity q fluid flux n porosity Dhyd hydraulic dispersion

Coupled effects Chemical reaction rate Phase change Material properties Thermal expansion Solid-Fluid in porous media Biological growth

Temperature and Chemical Rxn Reaction Rate Constant Function Arrhenius eq EA: activation energy for reaction R: gas constant T: temperature A: Max rate term

Including phase change Internal Energy (J/m3) Temperature solid liquid vapor Area under curve = latent heat Cp(E/(kg3q)) Temperature (q)

Fluid properties Viscosity Density Thermal Conductivity Cp(E/(kg3q)) Temperature (q)

Thermal expansion Volumetric Linear

Solid Phase in Porous Media Tf Ts Heat loss by fluid Heat balance between fluid and solid

Material Properties https://docs.google.com/viewer?url=http%3A%2F%2Fwww.bakker.org%2Fdartmouth06%2Fengs150%2F13-heat.pdf

Heat Transfer by Radiation and Convection

Conceptual Model Radiation and convection Radiation and convection

U-tube Heat Exchanger Installation of a U-tube in a borehole Two pipes from a U-tube heat exchanger in a borehole U-tube heat exchanger Array of U-tube heat exchangers

Free Convection Rayleigh-Bernard Convection Cells

Convection in the Earth and Atm

Experiment cooling at the top Simulated lake http://www.sciencedirect.com/science/article/pii/S0894177707001409

Rayleigh number Onset of natural convection depends on Ra For a layer with a free top surface: Racrit=1100

Coefficient of Thermal Expansion

Effect of varying temperature on mixing in surface water