Oxygenlight

Oxygenlight is a term used to describe the faint, blue-green glow that can sometimes be observed in the night sky. This phenomenon is caused by the interaction of solar radiation with Earth's atmosphere. During the day, the sun emits a wide spectrum of light, including ultraviolet (UV) radiation. When this UV light reaches the Earth's atmosphere, it excites oxygen molecules, causing them to emit a faint glow. This glow is typically too dim to be seen with the naked eye during the day, but it becomes visible at night when the sun is below the horizon and the sky is dark. The oxygenlight is most commonly observed in the upper atmosphere, at altitudes of around 90-100 kilometers, where the air is thin and the conditions are right for this type of luminescence. It is a natural optical phenomenon that has been studied by scientists to better understand the Earth's atmosphere and the processes that occur within it.