Scattering of solar radiation

In summary, the visible scattering optical depth of the thin haze layer composed of hydrated aerosols with a diameter of 0.2 µm is 0.69. This value was calculated using the transmissivity equation, assuming non-absorbing aerosols and a sun directly overhead (θ = 0).
  • #1
Lara001
1
0

Homework Statement



A thin haze layer overlies the ground and is composed of hydrated aerosols of 0.2 micron (µm) diameter. It scatters 50% of sunlight incident upon it when the sun is directly overhead.

a) What is the visible scattering optical depth of the layer?


Homework Equations



I'm not sure about what formula to use, but with the information given, i thought :


sigma = optical depth

t (transmissivity) = exp(-sigma*sec(theta))


The Attempt at a Solution



theta = 0
transmissivity = 1/2 ( as 50% isn't scattered, and I am assuming no absorption, though, it wasn't stated)

solving for sigma

sigma = 0.69 (2.d.p)
 
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  • #2


Good job on using the transmissivity equation to solve for the optical depth! Your solution is correct, assuming that the haze layer is composed of non-absorbing aerosols and that the sun is directly overhead (θ = 0). Keep in mind that the optical depth (σ) is a dimensionless quantity, so it doesn't have units. Also, it's good practice to state your final answer with the correct number of significant figures, so the optical depth would be 0.69 (not 0.69 with 2 decimal places). Great work!
 

1. What is the scattering of solar radiation?

The scattering of solar radiation is the process by which particles in the Earth's atmosphere, such as molecules and aerosols, reflect or redirect incoming solar radiation in all directions. This results in the diffuse sunlight that we see during the day.

2. Why does solar radiation scatter?

Solar radiation scatters due to the interaction between sunlight and particles in the Earth's atmosphere. This interaction causes the sunlight to change direction and spread out in all directions, resulting in the scattering of solar radiation.

3. How does the scattering of solar radiation affect the Earth's climate?

The scattering of solar radiation plays a crucial role in regulating the Earth's climate. It helps to distribute solar energy across the planet, affecting temperature and precipitation patterns. It also contributes to the Earth's energy balance and affects the amount of heat trapped in the atmosphere.

4. What factors influence the scattering of solar radiation?

The scattering of solar radiation is influenced by several factors, including the size and composition of the scattering particles, the angle and intensity of the incoming sunlight, and the properties of the atmosphere such as density and humidity.

5. How is the scattering of solar radiation measured?

The scattering of solar radiation can be measured using various instruments, such as spectrophotometers, radiometers, and lidars. These instruments measure the amount of light scattered in different directions and can provide valuable data on the scattering properties of the atmosphere.

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