cirwin
Registered
here's the rundown on the green flash:
Although the sun appears yellow, it actually emits light of all wavelengths (red, orange, green, blue, ultraviolet, etc.). Each of these wavelengths of light is refracted slightly differently (in physics parlance, each wavelength has a different index of refraction). When sunlight is passed through raindrops, the difference in the way each color bends has the effect of spreading the light out into the familiar rainbow. The spreading of the light due to the differences in refractive index is called dispersion. Due to the angle of the sun and the amount of atmosphere it has to travel through, we normally don't notice this from sunlight. At sunset, however, the amount of atmosphere that the sunlight travels through is large enough such that the dispersion becomes apparent at the fringes of the sun. Therefore, at sunrise or sunset (when we see the edge of the sun), we can sometimes see the light split into its component colors. This would normally look like several rainbow-colored crescent slivers of the sun but, as I mentioned in my previous post, the short wavelengths (blue and violet) tend to get scattered by the atmosphere and do not come straight through to the eye. This leaves green as the next color to be seen, and it appears slightly above the red disc of the sun (since green bends by a different amount). This is the so-called green flash and it only lasts as long as it takes for enough sun to set (or rise) so that we aren't just seeing a fringe of the sun.
I hope this makes sense!
Although the sun appears yellow, it actually emits light of all wavelengths (red, orange, green, blue, ultraviolet, etc.). Each of these wavelengths of light is refracted slightly differently (in physics parlance, each wavelength has a different index of refraction). When sunlight is passed through raindrops, the difference in the way each color bends has the effect of spreading the light out into the familiar rainbow. The spreading of the light due to the differences in refractive index is called dispersion. Due to the angle of the sun and the amount of atmosphere it has to travel through, we normally don't notice this from sunlight. At sunset, however, the amount of atmosphere that the sunlight travels through is large enough such that the dispersion becomes apparent at the fringes of the sun. Therefore, at sunrise or sunset (when we see the edge of the sun), we can sometimes see the light split into its component colors. This would normally look like several rainbow-colored crescent slivers of the sun but, as I mentioned in my previous post, the short wavelengths (blue and violet) tend to get scattered by the atmosphere and do not come straight through to the eye. This leaves green as the next color to be seen, and it appears slightly above the red disc of the sun (since green bends by a different amount). This is the so-called green flash and it only lasts as long as it takes for enough sun to set (or rise) so that we aren't just seeing a fringe of the sun.
I hope this makes sense!