Jean Baptiste Joseph Fourier

Jean Baptiste Joseph Fourier (March 21, 1768  May 16, 1830) was a French mathematician and physicist who is best known for initiating the investigation of Fourier series and their application to problems of heat flow. The Fourier transform is also named in his honor.
He was born at Auxerre in the Yonne département of France, the son of a tailor, and was educated by the Benedictines. The commissions in the scientific corps of the army were reserved for those of good birth, and being thus ineligible he accepted a military lectureship on mathematics. He took a prominent part in his own district in promoting the revolution, and was rewarded by an appointment in 1795 in the École Normale Supérieure, and subsequently by a chair at the École Polytechnique.
Fourier went with Napoleon on his Eastern expedition in 1798, and was made governor of Lower Egypt. Cut off from France by the English fleet, he organized the workshops on which the French army had to rely for their munitions of war. He also contributed several mathematical papers to the Egyptian Institute which Napoleon founded at Cairo, with a view of weakening English influence in the East. After the British victories and the capitulation of the French under General Menou in 1801, Fourier returned to France, and was made prefect of Isère, and it was while there that he made his experiments on the propagation of heat. He moved to Paris in 1816. In 1822 he published his Théorie analytique de la chaleur, in which he bases his reasoning on Newton's law of cooling, namely, that the flow of heat between two adjacent molecules is proportional to the extremely small difference of their temperatures. In this work he claims that any functions of a variable, whether continuous or discontinuous, can be expanded in a series of sines of multiples of the variable  this result isn't correct at all. But the fact that some discontinuous functions are the sum of infinite series was a breakthrough. The question of determining when a function is the sum of its Fourier series has been fundamental for centuries. Lagrange had given particular cases of this (false) theorem, and had implied that the method was general, but he had not pursued the subject. Dirichlet was the first to give a satisfactory demonstration of it, with some restrictive conditions.
Fourier left an unfinished work on determinate equations which was edited by Claude Navier, and published in 1831; this contains much original matter, in particular there is a demonstration of Fourier's theorem on the position of the roots of an algebraic equation. Lagrange had shown how the roots of an algebraic equation might be separated by means of another equation whose roots were the squares of the differences of the roots of the original equation. François Budan, in 1807 and 1811, had enunciated the theorem generally known by the name of Fourier, but the demonstration was not altogether satisfactory. Fourier's proof is the same as that usually given in textbooks on the theory of equations. The final solution of the problem was given in 1829 by Jacques Charles François Sturm (18031855).
Fourier is also credited with the discovery in his essay in 1824 that gases in the atmosphere might increase the surface temperature of the Earth. This was the effect that would later be called the greenhouse effect. He established the concept of planetary energy balance. That planets obtain energy from number of sources that causes temperature increase. Planets also lose energy by infrared radiation (that Fourier called "chaleur obscure" or "dark heat") with the rate increasing with temperature. Therefore some temperature balance is reached. And atmosphere shifts the balance toward the higher temperatures due to consumption of radiation. Fourier recognized that Earth primarily gets energy from Sun radiation for which atmosphere is transparent and that internal Earth heat doesn't contribute much to the energy balance. However he incorrectly believed that there is a significant contribution of radiation from interplanetary space. Fourier reported on an experiment by M. de Saussure with a black box exposed to the Sun, and in which if thin glass is put on top of the box the temperature inside of the box increases [1] (http://www.wmconnolley.org.uk/sci/fourier_1827/fourier_1827.html#text). Infrared radiation was only discovered by Frederick Herschel 25 years later. Fourier understood that rate of infrared radiation increases with temperature but exact form of this dependency StefanBoltzmann law (fourthpower law) was only discovered 50 years later.
He died in Paris.
See also
Reference
 Initial text from the public domain Rouse History of Mathematics
 Fourier, J.B.J. Mémoires d l'Académie Royale des Sciences de l'Institute de France VII. 570604 (1827) (greenhouse effect essay)
External links
 Template:MacTutor Biography
 Fourier 1827: MEMOIRE sur les temperatures du globe terrestre et des espaces planetaires (http://www.wmconnolley.org.uk/sci/fourier_1827/fourier_1827.html)
Preceded by: PierreÉdouard Lémontey  Seat 5 Académie française  Succeeded by: Victor Cousin 
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