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Named after Johann Balmer, who discovered the Balmer formula, an empirical equation to predict the Balmer series, in 1885. Balmer lines are historically referred to as " H-alpha ", "H-beta", "H-gamma" and so on, where H is the element hydrogen. [ 10 ]
would be seen as a large, very bright bluish disk of 35° apparent diameter −37.42 star Betelgeuse: seen from 1 AU away −30.30: star Sirius A: seen from 1 AU away −29.30: star Sun: seen from Mercury at perihelion: −27.40: star Sun: seen from Venus at perihelion −26.832: star Sun: seen from Earth [16] about 400,000 times as bright as ...
The Balmer series is calculated using the Balmer formula, an empirical equation discovered by Johann Balmer in 1885. The visible spectrum of light from hydrogen displays four wavelengths , 410 nm , 434 nm, 486 nm, and 656 nm, that correspond to emissions of photons by electrons in excited states transitioning to the quantum level described by ...
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The luminous intensity (in candelas) is a measure of how bright the beam in a particular direction is. If a lamp has a 1 lumen bulb and the optics of the lamp are set up to focus the light evenly into a 1 steradian beam, then the beam would have a luminous intensity of 1 candela.
The relativistic Breit–Wigner distribution (after the 1936 nuclear resonance formula [1] of Gregory Breit and Eugene Wigner) is a continuous probability distribution with the following probability density function, [2]
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