Josef Stefan and his equation for infrared radiation
The fact that the thermoradiative wattage output per surface area power flux of a hot object, \(q\), is proportional to 4th power of its temperature was deduced by a German physicist named Josef Stefan in 1879 1879 is quite eventful in physics because it was the year when Maxwell passed away and Rayleigh took over the Cavendish chair, it was also the year when Einstein was born. It was also the year when Karl Pearson took his Tripos exam and placed third Wrangler. Many years later when the 23-year-old Einstein started the Olympia group in 1902, his first reading suggestion was Pearson's The Grammar of Science. : $$q \propto T^4$$ Stefan's proportionality was inspired by a certain infrared emission The explanation given by Tyndall in 1864 was: . . . 13 a spiral of platinum wire suitably supported was placed within the camera of the electric lamp at the place usually occupied by the carbon points. This spiral was connected with a v