Chapter 4: Problem 6
What is the \(d^{2}\)-law for droplet evaporation? What are the assumptions that have to be satisfied for this law to be valid?
Chapter 4: Problem 6
What is the \(d^{2}\)-law for droplet evaporation? What are the assumptions that have to be satisfied for this law to be valid?
All the tools & learning materials you need for study success - in one app.
Get started for freeThere is currently substantial interest in utilizing eukaryotic algae for the renewable production of several bioenergy carriers, including starches for alcohols, lipids for diesel fuel surrogates, and hydrogen for fuel cells. Algae can convert solar energy into fuels at high photosynthetic efficiencies and can thrive in saltwater systems. Part of an energy balance analysis of such a process is the computation of the penetration of the radiative heat flux in a pool of water. a. Considering the surface of the sun as a black surface at a temperature of 5777 \(\mathrm{K}\), determine the total (i.e., integrated over all wavelengths) solar heat flux incident on the top of the Earth's atmosphere. The radius of the sun is \(6.96 \times 10^{8} \mathrm{~m}\), and a representative value of the sun-to-Earth distance is \(1.496 \times 10^{11} \mathrm{~m}\). Compare your result to the generally accepted annual mean value of \(1366 \mathrm{~W} \cdot \mathrm{m}^{-2}\) and discuss possible reasons for difference. b. Assuming that at a certain location and time, when the sun is in the zenith, the total heat flux arriving on the Earth surface is \(1100 \mathrm{~W} \cdot \mathrm{m}^{-2}\), calculate the balance between incoming and outgoing radiative heat flux at the surface of a pond of stagnant water when the sun is at an angle of \(30^{\circ}\) from the zenith. The total hemispherical emissivity of water is known to vary from \(0.95\) to \(0.963\) in the temperature range from 273 to \(373 \mathrm{~K}\) (Kaviany, 2002 ). c. The absorption coefficient \(\mathbf{\kappa}_{\lambda}\) of clear water is known to depend on wavelength. In the visible range \((0.4-0.7 \mu \mathrm{m})\), it varies from \(0.02\) to \(0.6 \mathrm{~m}^{-1}\) (Modest 2003, p. 416 ). By solving the radiative transfer equation, determine the decrease of intensity of incoming sunlight in a water layer with a depth \(0.1 \mathrm{~m}\) for the case that the sun is at an angle of \(30^{\circ}\) from the zenith.
Equation (4.8) is valid when the heat conductivity is independent on the direction. How would a generalization look like for the case of heat conductivity being different in the three coordinate directions? Which physical properties, e.g., of biomass material, could cause such difference?
Explain in what sense the set of equations Equation (4.11) provides a solution for the surface-to-surface radiative heat transfer problem. How would you solve the equations (a) in the case that the temperature of all surfaces is known and (b) in the case that for some surfaces the temperature and for other surfaces the heat flux are known?
What is the difference between the infinite conductivity model and the finite conductivity model for fuel droplet evaporation?
Give examples of radiative heat transfer processes dominated by surface- tosurface transfer and of processes for which the effects of absorption and emission in the space between surfaces (participating medium) are essential.
What do you think about this solution?
We value your feedback to improve our textbook solutions.