Sunlight refraction at sunset at different latitudes?

In summary, the angle of incidence of sunlight decreases as one moves away from the equator. This is due to the fact that the path of sunlight is longer in higher latitudes.
  • #1
Mohsin03129
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“Sunlight due to refraction is greater in higher latitudes than at the equator because of shallower angles of incidence to horizon. It takes longer for Sun to go down half a degree at sunset at shallower angles.”

When I draw a diagram of sun rays incident towards the earth, the angle appears to be the same at the equator and say at 60 degrees latitude Due to corresponding angles.

Can someone explain this statement / what am I missing ?
 
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  • #2
Did you take into account that the Earth is a ball? The path through the atmosphere is longer at high latitudes.
 
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  • #3
mathman said:
Did you take into account that the Earth is a ball? The path through the atmosphere is longer at high latitudes.
I understand this. That sounds like a different reasoning than the “shallow angle “ one though?
 
  • #4
Shallow angle leads to longer path through atmosphere.
 
  • #5
mathman said:
Shallow angle leads to longer path through atmosphere.
mathman said:
Shallow angle leads to longer path through atmosphere.
thanks, what is the best way to visualise this angle of incidence?
Is it steeper at the equator?
 
  • #6
Outside of the equatorial zone, it is generally steeper at the equator than at higher latitudes.
 
  • #7
Path of sunlight is the same. Path of Sun in sky is different.
At the same latitude, the sunlight due to refraction varies due to season due to the path of Sun varying.
On equator, at equinox, Sun falls vertically from horizon to nadir, 90 degrees below horizon; at a solstice, it falls just 66 degrees below horizon. Sun on its way to travel from horizon to 90 degrees below in 6 hours spends less time between horizon and half a degree than Sun on its way from horizon to culminate 66 degrees below in 6 hours.
 
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  • #8
The only way I see the angle shallowing is if I draw a sun with parallel rays hitting earth.
The angle made by the ray with the normal to a tangent at any n-s point on the Earth surface gets shallower with increasing latitude. But surely normal to a tangent isn’t the horizon!?

I am actually not sure about the definition of Horizon here.. I was imagining the horizon to lie on the East West latitude line and the angle of incidence shouldn't change with this horizon.
 
  • #9
Parallel rays are what happens. the Earth's diameter is around 9000 miles, while the sun is around 93 million miles away.
 
  • #10
mathman said:
Parallel rays are what happens. the Earth's diameter is around 9000 miles, while the sun is around 93 million miles away.
Yes I know that
 
  • #11
snorkack said:
Path of sunlight is the same. Path of Sun in sky is different.
At the same latitude, the sunlight due to refraction varies due to season due to the path of Sun varying.
On equator, at equinox, Sun falls vertically from horizon to nadir, 90 degrees below horizon; at a solstice, it falls just 66 degrees below horizon. Sun on its way to travel from horizon to 90 degrees below in 6 hours spends less time between horizon and half a degree than Sun on its way from horizon to culminate 66 degrees below in 6 hours.
snorkack said:
Path of sunlight is the same. Path of Sun in sky is different.
At the same latitude, the sunlight due to refraction varies due to season due to the path of Sun varying.
On equator, at equinox, Sun falls vertically from horizon to nadir, 90 degrees below horizon; at a solstice, it falls just 66 degrees below horizon. Sun on its way to travel from horizon to 90 degrees below in 6 hours spends less time between horizon and half a degree than Sun on its way from horizon to culminate 66 degrees below in 6 hours.
Are you referring to the northern horizon here?
 
  • #12
Mohsin03129 said:
Are you referring to the northern horizon here?
A diagram of these angles would be useful
snorkack said:
Path of sunlight is the same. Path of Sun in sky is different.
At the same latitude, the sunlight due to refraction varies due to season due to the path of Sun varying.
On equator, at equinox, Sun falls vertically from horizon to nadir, 90 degrees below horizon; at a solstice, it falls just 66 degrees below horizon. Sun on its way to travel from horizon to 90 degrees below in 6 hours spends less time between horizon and half a degree than Sun on its way from horizon to culminate 66 degrees below in 6 hours.
when you say degrees below horizon , is that from the normal to a horizon?
 

1. What causes sunlight to appear red during sunset?

During sunset, sunlight has to travel through a longer path in the atmosphere before reaching our eyes. This causes the shorter blue and green wavelengths to scatter, leaving the longer red wavelengths to reach our eyes, giving the appearance of a red sun.

2. Why does the angle of sunlight change during sunset at different latitudes?

The angle of sunlight changes during sunset at different latitudes because of the Earth's tilt on its axis. At higher latitudes, the tilt causes the sun to appear lower in the sky, resulting in a longer path for the sunlight to travel through the atmosphere.

3. How does refraction affect the appearance of the sun at sunset?

Refraction is the bending of light as it passes through different mediums. As sunlight travels through the Earth's atmosphere, it encounters different layers of air with varying densities. This causes the sunlight to bend and appear distorted, giving the sun a unique appearance during sunset.

4. Is the refraction of sunlight at sunset the same at all latitudes?

No, the refraction of sunlight at sunset is not the same at all latitudes. As mentioned earlier, the Earth's tilt on its axis causes the angle of sunlight to change at different latitudes, resulting in variations in the amount of refraction and the appearance of the sunset.

5. How does the atmosphere affect the refraction of sunlight at sunset?

The Earth's atmosphere plays a crucial role in the refraction of sunlight at sunset. The different layers of air with varying densities cause the sunlight to bend and scatter, resulting in the unique colors and appearance of the sunset. The composition of the atmosphere, such as the amount of dust and pollutants, can also affect the refraction of sunlight at sunset.

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