

Fourier recognized the possibility that the Earth’s atmosphere might act as an insulator of some kind.

Curated/Reviewed by Matthew A. McIntosh
Public Historian
Brewminate
Introduction
Jean-Baptiste Joseph Fourier[1] (March 1768 โ 16 May 1830) was a French mathematician andย physicistย born inย Auxerreย and best known for initiating the investigation ofย Fourier series, which eventually developed intoย Fourier analysisย andย harmonic analysis, and their applications to problems ofย heat transferย andย vibrations. Theย Fourier transformย andย Fourier’s law of conductionย are also named in his honour. Fourier is also generally credited with the discovery of theย greenhouse effect.[2]
Biography
Fourier was born inย Auxerreย (now in theย Yonneย dรฉpartementย of France), the son of aย tailor. He wasย orphanedย at the age of nine. Fourier was recommended to theย Bishop of Auxerreย and, through this introduction, he was educated by theย Benedictine Orderย of the Convent of St. Mark. 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 theย French Revolution, serving on the local Revolutionary Committee. He was imprisoned briefly during theย Terrorย but, in 1795, was appointed to theย รcole Normaleย and subsequently succeededย Joseph-Louis Lagrangeย at theย รcole Polytechnique.
Fourier accompaniedย Napoleon Bonaparteย on hisย Egyptian expeditionย in 1798, as scientific adviser, and was appointed secretary of theย Institut d’รgypte. Cut off from France by the British 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 (also called the Cairo Institute) which Napoleon founded atย Cairo, with a view of weakening British influence in the East. After the British victories and the capitulation of the French underย General Menouย in 1801, Fourier returned to France.

In 1801,[4]ย Napoleonย appointed Fourierย Prefectย (Governor) of theย Department of Isรจreย inย Grenoble, where he oversaw road construction and other projects. However, Fourier had previously returned home from the Napoleon expedition to Egypt to resume his academic post as professor atย รcole Polytechniqueย whenย Napoleonย decided otherwise in his remark
… the Prefect of the Department of Isรจre having recently died, I would like to express my confidence in citizen Fourier by appointing him to this place.[4]

Hence being faithful to Napoleon, he took the office of Prefect.[4]ย It was while at Grenoble that he began to experiment on the propagation of heat. He presented his paperย On the Propagation of Heat in Solid Bodiesย to the Paris Institute on 21 December 1807. He also contributed to the monumentalย Description de l’รgypte.[5]
In 1822, Fourier succeededย Jean Baptiste Joseph Delambreย as Permanent Secretary of theย French Academy of Sciences. In 1830, he was elected a foreign member of theย Royal Swedish Academy of Sciences.
Fourier never married.[6]
In 1830, his diminished health began to take its toll:
Fourier had already experienced, in Egypt and Grenoble, some attacks ofย aneurysmย of the heart. At Paris, it was impossible to be mistaken with respect to the primary cause of the frequent suffocations which he experienced. A fall, however, which he sustained on the 4th of May 1830, while descending a flight of stairs, aggravated the malady to an extent beyond what could have been ever feared.[7]
Shortly after this event, he died in his bed on 16 May 1830.

Fourier was buried in theย Pรจre Lachaise Cemeteryย in Paris, a tomb decorated with an Egyptian motif to reflect his position as secretary of the Cairo Institute, and his collation ofย Description de l’รgypte. His name is one of theย 72 names inscribed on the Eiffel Tower.
A bronze statue was erected in Auxerre in 1849, but it was melted down for armaments during World War II.[a]ย Joseph Fourier Universityย in Grenoble was named after him.
‘The Analytic Theory of Heat’

In 1822, Fourier published his work onย heat flowย inย Thรฉorie analytique de la chaleurย (The Analytical Theory of Heat),[8]ย in which he based his reasoning onย 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. This book was translated,[9]ย with editorial ‘corrections’,[10]ย into English 56 years later by Freeman (1878).[11]ย The book was also edited, with many editorial corrections, byย Darbouxย and republished in French in 1888.[10]
There were three important contributions in this work, one purely mathematical, two essentially physical. In mathematics, Fourier claimed that any function of a variable, whetherย continuousย orย discontinuous, can be expanded in a series ofย sinesย of multiples of the variable. Though this result is not correct without additional conditions, Fourier’s observation that some discontinuous functions are the sum of infinite series was a breakthrough. The question of determining when a Fourier series converges has been fundamental for centuries.ย Joseph-Louis Lagrangeย had given particular cases of this (false) theorem, and had implied that the method was general, but he had not pursued the subject.ย Peter Gustav Lejeune Dirichletย was the first to give a satisfactory demonstration of it with some restrictive conditions. This work provides the foundation for what is today known as theย Fourier transform.
One important physical contribution in the book was the concept ofย dimensional homogeneityย in equations; i.e. an equation can be formally correct only if the dimensions match on either side of the equality; Fourier made important contributions toย dimensional analysis.[12]ย The other physical contribution was Fourier’s proposal of hisย partial differential equationย for conductive diffusion of heat. This equation is now taught to every student of mathematical physics.
Real Roots of Polylnomials

Fourier left an unfinished work on determining and locating real roots of polynomials, which was edited byย Claude-Louis Navierย and published in 1831. This work contains much original matterโin particular,ย Fourier’s theorem on polynomial real roots, published in 1820. Fourier’s theorem on real roots of polynomials states that a polynomial with real coefficients has a real root between any two consecutive zeros of its derivative.[13][14]
Franรงois Budan, in 1807 and 1811, had published independently hisย theoremย (also known by the name of Fourier), which is very close to Fourier’s theorem (each theorem is a corollary of the other). Fourier’s proof[13]ย is the one that was usually given, during 19th century, in textbooks on the theory of equations.[b]ย Aย complete solution of the problemย was given in 1829 byย Jacques Charles Franรงois Sturm.[15]
Discovery of the Greenhouse Effect

In the 1820s, Fourier calculated that an object the size of the Earth, and at its distance from the Sun, should be considerably colder than the planet actually is if warmed by only the effects of incoming solar radiation. He examined various possible sources of the additional observed heat in articles published in 1824[16]ย and 1827.[17]ย However, in the end, because of the large 33-degree difference between his calculations and observations, Fourier mistakenly believed that there is a significant contribution of radiation from interstellar space. Still, Fourier’s consideration of the possibility that the Earth’s atmosphere might act as an insulator of some kind is widely recognized as the first proposal of what is now known as theย greenhouse effect,[18]ย although Fourier never called it that.[19][20]
In his articles, Fourier referred to an experiment byย de Saussure, who lined a vase with blackened cork. Into the cork, he inserted several panes of transparent glass, separated by intervals of air. Midday sunlight was allowed to enter at the top of the vase through the glass panes. The temperature became more elevated in the more interior compartments of this device. Fourier noted that if gases in the atmosphere could form a stable barrier like the glass panes they would have a similar effect on planetary temperatures.[17]ย This conclusion may have contributed to the later use of the metaphor of the “greenhouse effect” to refer to the processes that determine atmospheric temperatures.[21]ย Fourier noted that the actual mechanisms that determine the temperatures of the atmosphere includedย convection, which was not present in de Saussure’s experimental device.
See endnotes and bibliography at source.
Originally published by Wikipedia, 10.03.2002, under a Creative Commons Attribution-ShareAlike 3.0 Unported license.


