Metadata
Author: WikiMatrix
Data
English[en]
In 1879, Jožef Stefan observed that the total radiant flux from a blackbody is proportional to the fourth power of its temperature and stated the Stefan–Boltzmann law.
Spanish[es]
In 1879, Jožef Stefan observando que el flujo radiante total a partir de un cuerpo negro es proporcional a la cuarta potencia de su temperatura y se indica la Ley de Stefan-Boltzmann.