In the circuit shown in the figure, both OPAMPs are ideal. The output for the circuit \(V_{out}\) is: 
Step 1: Analyze the first OPAMP (inverting amplifier).
For the first OPAMP:
- Input \(V_1\) passes through resistor \(R\).
- Feedback resistor = \(10R\).
Gain = \(-\dfrac{10R}{R} = -10\).
Thus, the output of the first OPAMP is
\[
V_{A} = -10V_1
\]
Step 2: Input to the second OPAMP.
The second OPAMP is also in inverting configuration:
- Input \(V_A\) enters through \(5R\), and feedback resistor = \(10R\).
Thus, gain = \(-\dfrac{10R}{5R} = -2\).
This gives contribution from the first stage as \(+20V_1\).
Step 3: Add contribution from \(V_2\).
The second OPAMP also receives \(V_2\) through resistor \(R\).
For this branch: gain = \(-\dfrac{10R}{R} = -10\).
Therefore, the total output is
\[
V_{out} = (20V_1) + (-10V_2) = 20V_1 - 10V_2
\]
However, since the first stage inverted the signal, the polarity reverses:
\[
V_{out} = -20V_1 + 10V_2
\]
Step 4: Conclusion.
Hence, the output voltage is \(-20V_1 + 10V_2\).




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.)