Previous (Chronologically) Next Biographies Index Previous ( Alphabetically) Next Welcome page
He showed empirically, in 1879, that total radiation from a blackbody is proportional to the fourth power of its absolute temperature. Boltzmann, one of his students, showed in 1884 that this Stefan-Boltzmann law could be demonstrated mathematically. Stefan then applied it to determine the approximate temperature of the surface of the Sun. He also did important work on heat conduction in fluids and the kinetic theory of heat.
References elsewhere in this archive:
Tell me about Stefan's work in Quantum Mechanics
References:
Previous (Chronologically) Next Biographies Index Previous ( Alphabetically) Next Welcome page History Topics Index Famous curves index Chronologies Birthplace Map Mathematicians of the day Anniversaries for the year Search Form Simple Search Form Search Suggestions