Thermal radiation

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This article/section is a stub — some half-sorted notes, not necessarily checked, not necessarily correct. Feel free to ignore, or tell me about it.


Thermal radiation

physics mostly uses uses this to to "if it is above 0 Kelvin, then it emits some electromagnetism"
in an everyday sense we mostly think about the heat component
https://en.wikipedia.org/wiki/Thermal_radiation



Black-body radiation is basically the same thing, but with a few more assumptions to formalize it, because thermal radiation's real-world math becomes easier if we add some assumptions such as

assuming a uniform temperature
assuming a uniform absorber of energy
(which also helps it have a smooth spectrum.)
assuming it's not really interacting in other ways
frequently assuming an object out in space, because the way we see it is affected largely by heat (and not also a mess of other things)
https://en.wikipedia.org/wiki/Black-body_radiation



Incandescence is also sort of the same thing -- but zoomed in to care only about the human-visible-light range of that EM emission

usually with a temperature between 500K (below which you don't see much) and 15000K (some xenon lamps? Practically the ~6000K sun is what we see most often)

In the context of lighting,

incandescent lightbulbs are wires that glow when given mains voltage, and continue glowing for a while.
incandescent lighting is perhaps mainly contrasted with luminescence, which is roughly the "light for any other reason" category (and contains a handful of specific reasons).
https://en.wikipedia.org/wiki/Incandescence



If you wanted a "all things that happen at high temperature" view, there are some further things to list, such as thermionic emission.