In the following circuit, $RC$ is much larger than the input period. Assume diode is ideal and $R$ is large. The dc output voltage across $R$ will be .............. V. (Specify answer up to one digit after the decimal point.) 
Step 1: Note that $RC \gg T$.
Thus capacitor charges to peak voltage and discharges very slowly — typical peak detector.
Step 2: Input is 24 Vrms.
Peak voltage = $24\sqrt{2} = 33.94\ \text{V}$.
Step 3: Ideal diode.
No drop across diode, so capacitor charges to full peak voltage.
Step 4: DC output across $R$.
Since discharge is negligible,
$V_{out} \approx V_{peak} = 33.94 \approx 34.0\ \text{V}$.




At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)