Derive an expression for the spectral energy density ρλ(λ)[the energy per unit volume in the wavelength region between λ and λ+dλ is ρλ(λ)dλ]. Show that the wavelength λp at which the spectral energy density is maximum satisfies the equation 5(1-e-y ) = y, where y=hc/λpkT, demonstrating that the relationship λpT = constant (Wien’s Law) is satisfied. Find λpT approximately. Show that λp ≠c/νp, where νp is the frequency at which the blackbody energy density ρv is maximum. The shapes and peak locations of density functions depend on the representation chosen.
Derive an expression for the spectral energy density ρλ(λ)[the energy per unit volume in the wavelength...
1. The solar energy spectral density is shown in the right figure. By assuming that the sun is a blackbody, use the Planck's distribution function to fit the extraterrestrial solar energy spectral density. Extraterrestrial (a) Determine the most possible surface temperature T of sun by fitting the Planck's distribution to the extraterrestrial solar energy spectral density. You can choose a few temperatures to see which temperature can best fit the peak (at Amsx) and the entire profile of the extraterrestrial...
Consider a cylindrical capacitor like that shown in Fig. 24.6. Let d = rb − ra be the spacing between the inner and outer conductors. (a) Let the radii of the two conductors be only slightly different, so that d << ra. Show that the result derived in Example 24.4 (Section 24.1) for the capacitance of a cylindrical capacitor then reduces to Eq. (24.2), the equation for the capacitance of a parallel-plate capacitor, with A being the surface area of...