Study Guide 1 Flashcards
(32 cards)
Heat Transfer
thermal energy in transit due to a spatial temperature difference
Heat flux
HT rate in the 1D direction per unit area perpendicular to the direction of transfer: W/m^2
Mass Transfer
Movement of mass due to a species/[ ] gradient in the mixture
Mass flux
MT rate in the 1D direction per unit area perpendicular to the direction of transfer: kg of A /m^2 s
Conduction
HT through a solid material or stagnant fluid: electron movement (HT)
Diffusion
MT through a solid material or stagnant fluid: random particle movements
Convection (Heat or Mass)
HT or MT between a surface and an adjacent fluid: movement of heat/mass by both conduction/diffusion and advection (bulk fluid motion)
Radiation
HT transfer by emission and absorption of incident electromagnetic radiation
Thermal conductivity
Transport property that is characteristic of the wall material: k = W/mK
Binary diffusion coefficient
D,AB used in Fick’s Law nd is a function of T/P: D,AB = m^2/s
Mass diffusivity
Another name for the binary diffusion coefficient
Fourier’s law
q” = -k (dT/dz)
Fick’s law
j, Az = -D,AB(dpa/dz)
Stationary medium approximation
1) small concentration
2) no advection/bulk fluid movement
What allows us to say that j = N for Fick’s Law and Diffusion
Newton’s law of cooling
For Convection, q” = h(Ts - T-infinity)
Heat transfer coefficient
h = W/m^2 K
Parameter NOT a property: depends on how fast the movement is
Mass Transfer coefficient
kc = m/s
Used in the mass equivalent of the Newton’s Law of Cooling Equation (n,a” = kc(ps - p-infinity) where p = density
Forced convection
when the flow is caused by external means like a fan, pump, or atmospheric winds
Free convection
When the flow is induced by buoyancy forces which are due to density differences caused by temperature variations in the fluid
Stefan - Boltzmann law
There is an upper limit to a surface’s emissivity power
Constant: 5.67 x 10^-8 W/m^2 K^4
q” net = Eo(Ts^4 - Tsurr^4)
E = epsilon, o = sigma
0 <= E <= 1
Blackbody
Where the surface emissivity is 1:
Eb = q” emitted = oTs^4
Gray body
q” rad = EoTs^4 - aG = Eo(Ts^4 - Tsurr^4)
where a = alpha; absorptivity (0-1)
Irradiation
The rate at which all such radiation is incident on a unit area of the surface (G)
Absorptivity
A surface radiative property based on the opaqueness of a surface:
Opaque: <1