|Monochromatic Atomic Lights
Peter Rosen imaged this at Östersund, Sweden. “We had a beautiful little aurora. There was plenty of fog so we had to find a spot higher up and away from the lake to get an almost free view. Behind us there were sodium streetlights with their typical amber color. The streetlights are the lightsource of the heiligenschein around my camera on the tripod.” Nearly all the light in the scene, except that from the stars, is narrow band atomic radiation. ©Peter Rosen, shown with permission
|The bound electron waves surrounding atoms can have only discrete energies. When an isolated atom is disturbed in some way, for example by a collision with a high energy particle, an electron wave can have its energy increased to another higher energy discrete state. To be pedantic, the higher energy state need not always be discrete for if the energy is high enough we have a free electron and an ionised atom.
The degree of monochromaticity is a key difference between street lamps and aurorae.
Street lamp tubes have reasonable pressures compared to the upper atmosphere and therefore have slightly radiation broadened light. Astronomer loathed high pressure sodium street lamps have such extensive pressure broadening that their sky polluting light cannot be filtered.
Auroral discharges are from (in Peter’s case) oxygen atoms in the near vacuum of the upper atmosphere disturbed by particles ejected from Earth’s magnetotail. Quantum mechanics rears its head in that the oxygen high energy state is awkward. Ordinary transitions back to the original low lower energy wave are not permitted because the electron spins of each condition are not compatible. But nearly all things happen in quantum mechanics. The electron energy eventually seeps away in the familiar auroral green glow. But ‘eventually’ is comparable to the age of the Universe in atomic terms. The Uncertainty Principle acts again. The time of the emission is grossly uncertain and its HUP pairing with the radiation bandwidth means that the green light has an extremely narrow wavelength spread.
|Sunlight has a near continuous spectrum. The original gamma radiation from the core is downgraded by endless energetic collisions on its long journey to the surface. The resulting pressure broadening produces a near thermal equilibrium 'black body' wavelength distribution. Only absorptions by atoms close to the solar surface mar this smooth spectrum.|