With the rapid development of many new and varied sources of light in the 19th century—Argand lamps of different designs and which burned various fuels, Carcel lamps, stearin candles, paraffin candles, and spermaceti candles, electric arc lamps, Drummond lamps, incandescent lamps with various filaments, Nernst glowbars, and many others —some method was needed to compare their output. But with the sources varying in spectral content and the angular distribution of the light, how could a meaningful comparison be made? After various fruitless attempts were made to concentrate the light onto a uniform region a surprisingly simple solution was proposed.