Rayleigh Scattering: Blue/Red Irradiance Ratio & Distance

In summary, the scattering irradiance ratio between blue and red does not change significantly with distance due to Rayleigh scattering. This is because even though blue light is scattered out more than red light, both colors still reach the observer with greater than 90% of their original intensity. However, when the sun is on the horizon, the light has to travel through a longer distance of about 100 miles, resulting in the appearance of a red or orange sun. This phenomenon can be explained by the fact that blue light has a shorter wavelength than red light.
  • #1
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Homework Statement
General question
Relevant Equations
I is prop to λ**(-4)
Hi everyone, does the scattering irradiance ratio between blue/red change with distance with Rayleigh scattering?
I would think that it would remain generally constant..
 
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  • #2
A little info that should provide some helpful hints: When the sun is overhead, the light has about 10-20 miles of atmosphere to go through to reach you. The blue light gets scattered out more than the red light, but for both colors through this relatively short distance, greater than 90% of the light reaches the observer. When the sun is on the horizon, the light from the sun goes through perhaps 100 miles or more of atmosphere to reach the observer, because the atmosphere is a thin ring of about 20 miles thickness, on the circular (spherical earth) with a radius of about 4000 miles. ## \\ ## That should explain why the sun appears red or orange in a sunset, but looks white when viewed overhead. If you do a little arithmetic logic with this info, it should provide the answer to your question.## \\ ## (Note: blue light has a wavelength approximately half that of red light).
 

FAQ: Rayleigh Scattering: Blue/Red Irradiance Ratio & Distance

1. What is Rayleigh scattering?

Rayleigh scattering is the phenomenon where light is dispersed or scattered by particles in the atmosphere, such as air molecules. This scattering is more prominent for shorter wavelengths, such as blue light, which is why the sky appears blue during the day.

2. What is the blue/red irradiance ratio and its significance?

The blue/red irradiance ratio is the ratio of the amount of blue light to the amount of red light that is scattered in the atmosphere. This ratio can vary depending on the distance between the source of light and the observer. It is significant because it can provide information about the atmosphere, such as its composition and density.

3. How does the blue/red irradiance ratio change with distance?

The blue/red irradiance ratio decreases as the distance between the source of light and the observer increases. This is because the amount of blue light scattered by the atmosphere decreases more rapidly with distance compared to red light. Therefore, the ratio of blue to red light decreases as the distance increases.

4. Can the blue/red irradiance ratio be used to determine the distance to a light source?

No, the blue/red irradiance ratio cannot be used to accurately determine the distance to a light source. Other factors, such as the angle of observation and the amount of particles in the atmosphere, can also affect the ratio. Therefore, it is not a reliable method for measuring distance.

5. How does Rayleigh scattering affect astronomy and remote sensing?

Rayleigh scattering plays a significant role in astronomy and remote sensing. By studying the blue/red irradiance ratio, scientists can gather information about the composition and density of planetary atmospheres. It also affects the colors we see in images taken from space, as different wavelengths of light are scattered differently by the atmosphere.

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