Solar Engineering of Thermal Processes (4th Edition) by John A. Duffie, William A. Beckman

By John A. Duffie, William A. Beckman

The up to date fourth variation of the "bible" of solar power thought and applications

Over a number of variations, Solar Engineering of Thermal Processes has turn into a vintage sun engineering textual content and reference. This revised Fourth Edition bargains present insurance of solar power idea, platforms layout, and functions in numerous marketplace sectors in addition to an emphasis on sunlight method layout and research utilizing simulations to aid readers translate conception into practice.
An very important source for college students of sun engineering, solar power, and replacement power in addition to pros operating within the strength and effort or similar fields, Solar Engineering of Thermal Processes, Fourth Edition features:• elevated insurance of modern issues similar to photovoltaics and the layout of sun cells and heaters
• A brand-new bankruptcy on making use of CombiSys (a readymade TRNSYS simulation application on hand at no cost obtain) to simulate a sun heated residence with sunlight- heated family scorching water
• extra simulation difficulties to be had via a spouse website
• an intensive array of homework difficulties and exercises

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Extra resources for Solar Engineering of Thermal Processes (4th Edition)

Example text

3 Calculate Rb for a latitude 40◦ N at a tilt of 50◦ toward the south for the hour 9 to 10 solar time on February 16. 45. To find cos θ , enter at an abscissa of +10◦ , using the curve for February 16 for south latitudes. 80. 78. 2, to construct plots showing the effects of collector tilt on Rb for various times of the year and day. 3 Ratio Rb for a surface with slope 50◦ to south at latitude 40◦ for various hours from solar noon. such a plot for a latitude of 40◦ and a slope of 50◦ . It illustrates that very large gains in incident beam radiation are to be had by tilting a receiving surface toward the equator.

A Take three points indicated by A, B, and C in the diagram with A to the south and B 10 m and C 30 m west of A. Points B and C are taken to the east of A with the same object altitude angles as B and C and with object azimuth angles changed only in sign. For point A, the object azimuth γoA is 0◦ . 6 ◦ There are points corresponding to B and C but to the east of A; these will have the same object azimuth angles except with negative signs. The shading profile determined by these coordinates is independent of latitude.

30 Solar Radiation trees, buildings, or other obstructions. The geometries may be irregular, and systematic calculations of shading of the receiver in question may be difficult. Recourse is made to diagrams of the position of the sun in the sky, for example, plots of solar altitude αs versus solar azimuth γs , on which shapes of obstructions (shading profiles) can be superimposed to determine when the path from the sun to the point in question is blocked. The second type includes shading of collectors in other than the first row of multirow arrays by the collectors on the adjoining row.

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