Question

The solar constant is the radiant flux density at a spherical surface centered on the Sun having a radius equal to that of the Earth's mean orbital radius; it has a value of $0.133-0.14 \mathrm{W} / \mathrm{cm}^{2}$. If we assume an average wavelength of about $700 \mathrm{nm}$, how many photons at most will arrive on each square meter per second of a solar cell panel just above the atmosphere?

Name: The solar constant is the radiant flux density at a spherical surface centered on the Sun having a radius equal to that of the Earth's mean orbital radius; it has a value of 0.133-0.14 W / cm^2. If we assume an average wavelength of about 700 nm, how many photons at most will arrive on each square meter per second of a solar cell panel just above the atmosphere?
Uploaded: 2022-04-12T11:52:05-08:00
Duration: 2 min 11 s
Channel: Yuva S
Description: The solar constant is the radiant flux density at a spherical surface centered on the Sun having a radius equal to that of the Earth's mean orbital radius; it has a value of 0.133-0.14 W / cm^2. If we assume an average wavelength of about 700 nm, how many photons at most will arrive on each square meter per second of a solar cell panel just above the atmosphere?

          The solar constant is the radiant flux density at a spherical surface centered on the Sun having a radius equal to that of the Earth's mean orbital radius; it has a value of $0.133-0.14 \mathrm{W} / \mathrm{cm}^{2}$. If we assume an average wavelength of about $700 \mathrm{nm}$, how many photons at most will arrive on each square meter per second of a solar cell panel just above the atmosphere?

Added by Eva N.

University Physics with Modern Physics

Hugh D. Young 14th Edition

Instant Answer

Solved by Expert Yuva S

04/12/2022

Step 1

Given: Average wavelength, $\lambda = 700 nm = 700 \times 10^{-9} m$ Speed of light, $c = 3 \times 10^8 m/s$ Energy of a photon, $E = \frac{hc}{\lambda}$, where $h$ is the Planck's constant. Plugging in the values, we get: $E = \frac{6.626 \times 10^{-34} J \cdot Show more…

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The solar constant is the radiant flux density at a spherical surface centered on the Sun having a radius equal to that of the Earth's mean orbital radius; it has a value of $0.133-0.14 \mathrm{W} / \mathrm{cm}^{2}$. If we assume an average wavelength of about $700 \mathrm{nm}$, how many photons at most will arrive on each square meter per second of a solar cell panel just above the atmosphere?