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<v Speaker 1>Chapter eighteen, Part four of A Short Account of the

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<v Speaker 1>History of Mathematics by W. W. Rowsball. This is a

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<v Speaker 1>LibriVox recording. All LibriVox recordings are in the public domain.

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<v Speaker 1>For more information or to volunteer, please visit LibriVox dot org.

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<v Speaker 1>This is a reading by Paul King PJK dot scripts

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<v Speaker 1>that I might t dot e d U forward slash

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<v Speaker 1>p j K. A Short account of the History of

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<v Speaker 1>mathematics by W. W. Rowsball, Chapter eighteen Leibniz and the

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<v Speaker 1>Mathematicians of the first half of the eighteenth century, Part four. Cavendish,

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<v Speaker 1>the Honorable Henry Cavendish was born at Nice on October tenth,

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<v Speaker 1>seventeen thirty one, and died in London on February twenty fourth,

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<v Speaker 1>eighteen ten. His tastes for scientific research and mathematics were

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<v Speaker 1>formed at Cambridge, where he resided from seventeen forty nine

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<v Speaker 1>to seventeen fifty three. He created experimental electricity and was

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<v Speaker 1>one of the earliest writers to treat chemistry as an

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<v Speaker 1>exact science. I mention him here on account of his

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<v Speaker 1>experiment in seventeen ninety eight to determine the density of

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<v Speaker 1>the Earth by estimating its attraction as compared with that

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<v Speaker 1>of two given lead balls. The result is that the

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<v Speaker 1>mean density of the Earth is about five and a

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<v Speaker 1>half times that of water. This experiment was carried out

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<v Speaker 1>in accordance with a suggestion which had been first made

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<v Speaker 1>by John Mitchell, a fellow of Queen's College, Cambridge, who

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<v Speaker 1>had died before he was able to carry it into effect. Rumford,

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<v Speaker 1>Sir Benjamin Thompson, Count Rumford, born at Concord on March

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<v Speaker 1>twenty sixth, seventeen fifty three and died at Auteil on

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<v Speaker 1>August twenty first, eighteen fifteen. Was of English descent and

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<v Speaker 1>fought on the side of the lawyer Illis in the

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<v Speaker 1>American War of Secession. On the conclusion of peace, he

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<v Speaker 1>settled in England, but subsequently entered the service of Bavaria,

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<v Speaker 1>where his military and civil powers of organization proved of

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<v Speaker 1>great value. At a later period he again resided in England,

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<v Speaker 1>and when there he founded the Royal Institution. The majority

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<v Speaker 1>of his papers were communicated to the Royal Society of London.

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<v Speaker 1>Of these, the most important is his memoir, in which

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<v Speaker 1>he shewed that heat and work are mutually convertible. Young.

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<v Speaker 1>Among the most eminent physicists of his time was Thomas Young,

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<v Speaker 1>who was born in Milverton on June thirteenth, seventeen seventy

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<v Speaker 1>three and died in London on May tenth, eighteen twenty nine.

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<v Speaker 1>He seems as a boy to have been somewhat of

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<v Speaker 1>a prodigy, being well read in modern languages and literature

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<v Speaker 1>as well as in science. He always kept up his

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<v Speaker 1>literary tastes, and it was he who first furnished the

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<v Speaker 1>key to decipher the Egyptian hieroglyphics. He was destined to

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<v Speaker 1>be a doctor, and after attending lectures at Edinburgh and Gottingen,

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<v Speaker 1>entered im Manual College, Cambridge, from which he took his

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<v Speaker 1>degree in seventeen ninety nine, and to his stay at

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<v Speaker 1>the university he attributed much of his future distinction. His

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<v Speaker 1>medical career was not particularly successful, and his favorable maxim

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<v Speaker 1>that a medical diagnosis is only a balance of probabilities

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<v Speaker 1>was not appreciated by his patients, who looked for certainty

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<v Speaker 1>and returned for their fee. Fortunately, his private means were ample.

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<v Speaker 1>Several papers contributed to various learned societies from seventeen ninety

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<v Speaker 1>eight onwards prove him to have been a mathematician of

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<v Speaker 1>considerable power. But the researches which have immortalized his name

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<v Speaker 1>are those by which he laid down the laws of

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<v Speaker 1>interference of waves and light, and was thus able to

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<v Speaker 1>suggest the means by which the chief difficulties in the

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<v Speaker 1>way of acceptance of the undulatory theory of light could

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<v Speaker 1>be overcome. Wallaston. Another experimental physicist of the same time

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<v Speaker 1>in school was William Hyde Wallaston, who was born at

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<v Speaker 1>Dereham on August sixth, seventeen sixty six and died in

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<v Speaker 1>London on December twenty second, eighteen twenty eight. He was

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<v Speaker 1>educated at Caius College, Cambridge, of which society he was

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<v Speaker 1>a fellow. Besides his well known chemical experiments, he has

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<v Speaker 1>celebrated for his researches on experimental optics and for the

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<v Speaker 1>improvements which he affected in astronomical instruments. Dalton. Another distinguished

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<v Speaker 1>writer of the same period was John Dalton, who was

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<v Speaker 1>born in Cumberland on September fifth, seventeen sixty six and

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<v Speaker 1>died at Manchester on July twenty seventh, eighteen forty four.

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<v Speaker 1>Dalton investigated the tension of vapors and the law of

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<v Speaker 1>the expansion of a gas under changes of temperature. He

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<v Speaker 1>also found the atomic theory in chemistry. It will be

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<v Speaker 1>gathered from these notes that the English school of physicists

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<v Speaker 1>at the beginning of this century were mostly concerned with

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<v Speaker 1>the experimental side of the subject, but in fact no

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<v Speaker 1>satisfactory theory could be formed without some similar careful determination

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<v Speaker 1>of the facts. The most eminent French physicists of the

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<v Speaker 1>same time were Fourier, Poissin Ampere, and Fresnol. Their method

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<v Speaker 1>of treating the subject is more mathematical than that of

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<v Speaker 1>their English contemporaries, and the two first named were distinguished

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<v Speaker 1>for general mathematical ability. Fourier. The first of these French

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<v Speaker 1>physicists was Jean Baptiste Joseph Fourier, who was born at

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<v Speaker 1>Auterre on March twenty first, seventeen sixty eight and died

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<v Speaker 1>at Paris on May sixteenth, eighteen thirty. He was the

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<v Speaker 1>son of a tailor and was educated by the Benedictines.

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<v Speaker 1>The commissions in the scientific corps of the army was,

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<v Speaker 1>as still the case in Russia, reserved for those of

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<v Speaker 1>good birth, and being thus ineligible, he accepted a military

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<v Speaker 1>lectureship on mathematics. He took a prominent part in his

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<v Speaker 1>own district in promoting the revolution, and was rewarded by

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<v Speaker 1>an appointment in seventeen ninety five in the normal school,

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<v Speaker 1>and subsequently by a chair at the Polytechnic School. He

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<v Speaker 1>went with Napoleon on his Eastern expedition in seventeen ninety

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<v Speaker 1>eight and was made governor of Lower Egypt, cut off

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<v Speaker 1>from France by the English fleet, he organized the workshops

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<v Speaker 1>on which the French army had to rely for their

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<v Speaker 1>munitions of war. He also contributed several mathematical papers to

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<v Speaker 1>the Agiat Institute, which Napoleon founded at Cairo with a

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<v Speaker 1>view of weakening English influence in the East. After the

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<v Speaker 1>British victories and the capitulation of the French under General

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<v Speaker 1>Manon in eighteen oh one, he returned to France and

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<v Speaker 1>was made prefect of Grenoble, and it was while there

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<v Speaker 1>that he made his experiments on the propagation of heat.

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<v Speaker 1>He moved to Paris in eighteen sixteen. In eighteen twenty

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<v Speaker 1>two he publishes Theory and a Letigue les chere, in

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<v Speaker 1>which he bases his reasoning on Newton's law of cooling,

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<v Speaker 1>namely that the flow of heat between two adjacent molecules

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<v Speaker 1>is proportional to the infinitely small difference of their temperatures.

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<v Speaker 1>He states that the theory demands that the temperatures of

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<v Speaker 1>stellar space should be between minus fifty degrees celsius and

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<v Speaker 1>minus sixty degrees celsius, a conclusion which it has been

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<v Speaker 1>as yet impossible to prove or disproof. In this work

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<v Speaker 1>issues that any function of a variable, whether continuous or discontinuous,

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<v Speaker 1>can be expanded in a series of signs of multiples

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<v Speaker 1>of the variable, a result which is constantly used in

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<v Speaker 1>modern analysis. Lagrange had given particular cases of the theorem

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<v Speaker 1>and had implied that the method was general, but he

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<v Speaker 1>had not pursued the subject. Fourier left an unfinished work

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<v Speaker 1>on determinate equations, which was edited by Navier and published

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<v Speaker 1>in eighteen thirty one. This contains much original matter. In particular,

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<v Speaker 1>there is a demonstration of Fourier's theorem on the position

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<v Speaker 1>of the roots of an algebraic equation. Lagrange had shown

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<v Speaker 1>how the roots of an algebraical equation might be separated

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<v Speaker 1>by means of another equation whose roots were the squares

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<v Speaker 1>of the differences of the roots of the original equation.

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<v Speaker 1>Budan in eighteen o seven and X eighteen eleven had

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<v Speaker 1>enunciated the theorem generally known by the name of Fourier,

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<v Speaker 1>but the demonstration was clumsy and not altogether satisfactory. Fourier's

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<v Speaker 1>proof is the same as that usually given in textbooks

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<v Speaker 1>on the theory of equations. The final solution of the

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<v Speaker 1>problem was given in eighteen twenty nine by Jacques Chain,

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<v Speaker 1>Francois Sturm Saudiq Calnou. Among Fourier's contemporaries who were interested

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<v Speaker 1>in the theory of heat, the most eminent was Saldi Calno,

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<v Speaker 1>son of the eminent geometrician mentioned previously. Saudi Calno was

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<v Speaker 1>born at Paris in seventeen ninety six and died there

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<v Speaker 1>of cholera in August eighteen thirty two. He was an

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<v Speaker 1>officer in the French army. In eighteen twenty four he

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<v Speaker 1>issued a short work entitled Reflection selepresence montris deu feu,

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<v Speaker 1>in which he attempted to determine in what way heat

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<v Speaker 1>produced its mechanical effect. He made the mistake of assuming

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<v Speaker 1>that heat was material, but his essay was the commencement

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<v Speaker 1>of the modern theory of thermodynamics. Poissant Semeon. Denis Poisson

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<v Speaker 1>born at Pithiviers on June twenty first, seventeen eighty one

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<v Speaker 1>and died at Paris on April twenty fifth, eighteen forty

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<v Speaker 1>is almost equally distinguished for his application of mathematics to

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<v Speaker 1>mechanics and to physics. His father had been a common soldier,

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<v Speaker 1>and on his retirement was given some small administrative post

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<v Speaker 1>in his native village. When the revolution broke out, he

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<v Speaker 1>appears to have assumed the government of the place, and,

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<v Speaker 1>being left undisturbed, became a person of some local importance.

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<v Speaker 1>The boy was put out to nurse, and he used

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<v Speaker 1>to tell how one day his father, coming to see him,

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<v Speaker 1>found that the nurse had gone out on pleasure bent

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<v Speaker 1>while she had left him suspended by a small cord

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<v Speaker 1>to a nail fixed in the wall. This, she explained,

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<v Speaker 1>was a necessary precaution to prevent him from perishing under

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<v Speaker 1>the teeth of the various animals and animicula that roamed

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<v Speaker 1>on the floor. Poissin used to add that his gymnastic

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<v Speaker 1>efforts carried him incessantly from one side to the other,

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<v Speaker 1>and it was thus in his tenderest infancy that he

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<v Speaker 1>commenced those studies on the pendulum that were there to

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<v Speaker 1>occupy so large a part of his mature age. He

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<v Speaker 1>was educated by his father and destined, much against his will,

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<v Speaker 1>to be a doctor. His uncle offered to teach him

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<v Speaker 1>the art, and began by making him prick the veins

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<v Speaker 1>of cabbage leaves with a lancet. When perfect in this

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<v Speaker 1>he was allowed to put on blisters, but in almost

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<v Speaker 1>the first case he did this by himself. The patient

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<v Speaker 1>died in a few hours, and though all the medical

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<v Speaker 1>practitioners of the place assured him that the event was

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<v Speaker 1>a very common one, he vowed he would have nothing

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<v Speaker 1>more to do with the profession. Returning home, he found

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<v Speaker 1>amongst the official papers sent to his father a copy

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<v Speaker 1>of the Questions set at the Polytechnic School, and at

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<v Speaker 1>once found his career. At the age of seventeen, he

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<v Speaker 1>entered the Polytechnic, and his abilities excited the interests of

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<v Speaker 1>Lagrange and Laplace, whose friendship he retained to the end

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<v Speaker 1>of their lives. A memoir on Finite Differences, which he

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<v Speaker 1>wrote when only eighteen, was reported on so favorably by

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<v Speaker 1>Legendre that it was ordered to be published in the

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<v Speaker 1>Recuere des Sevante et cage. Directly he had finished the course,

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<v Speaker 1>he was made a lecturer at the school, and he

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<v Speaker 1>continued through his life to hold various government, scientific posts

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<v Speaker 1>and professorships. He was somewhat of a socialist, and remained

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<v Speaker 1>a rigid Republican till eighteen fifteen. With a view to

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<v Speaker 1>me making another empire impossible, he joined the Legitimists. He took, however,

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<v Speaker 1>no active part in politics, and made the study of

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<v Speaker 1>mathematics his amusement as well as his business. His works

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<v Speaker 1>and memoirs are between three and four hundred in number.

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<v Speaker 1>The chief treatises which he wrote were as Treates de

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<v Speaker 1>Mechanique two volumes, eighteen eleven and eighteen thirty three, which

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<v Speaker 1>was long a standard work, His Theory nouver de laxion

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<v Speaker 1>Capelli in eighteen thirty one, his Theory mathematic de lecheur

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<v Speaker 1>in eighteen thirty five, to which a supplement was added

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<v Speaker 1>in eighteen thirty seven, and is recherche les probability de

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<v Speaker 1>jugement in eighteen thirty seven. He had intended, if he

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<v Speaker 1>had lived, to write a work which should cover all

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<v Speaker 1>mathematical physics, and in which these would have been incorporated

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<v Speaker 1>of his memoirs on the subject of pure mathematics, the

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<v Speaker 1>most important are those on definite integrals and the Fourier's series.

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<v Speaker 1>These are to be found on the Jenel Polytechnique from

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<v Speaker 1>eighteen thirteen to eighteen twenty three and in the Memoir

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<v Speaker 1>de Lacademie for eighteen twenty three. Their application to physical

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<v Speaker 1>problems constituting one of his chief claims to distinction his

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<v Speaker 1>essay on the Calculus of variations Mamou de Lacademie eighteen

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<v Speaker 1>thirty three and his papers on the Probability of the

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<v Speaker 1>mean results of observations Connaissance de Tempe eighteen twenty seven

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<v Speaker 1>and following years. Most of his memoirs were published in

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<v Speaker 1>the three periodicals here mentioned. Perhaps the most remarkable of

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<v Speaker 1>his memoirs and applied mathematics are those on the theory

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<v Speaker 1>of electrostatics and magnetism, which originated a new branch of

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<v Speaker 1>mathematical physics. He supposed that the results were due to

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<v Speaker 1>the attractions and repulsions of imponderable part of the most

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<v Speaker 1>important of those on physical astronomy are the two re

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<v Speaker 1>read in eighteen oh six printed in eighteen oh nine

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<v Speaker 1>on the secular inequalities of the mean motions of the planets,

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<v Speaker 1>and on the variations of arbitrary constants introduced into the

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<v Speaker 1>solutions of questions on mechanics. In those Poissan discusses the

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<v Speaker 1>question of the stability of the planetary orbits, which Legendre

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<v Speaker 1>had already proved to the first degree of approximation for

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<v Speaker 1>the distributing forces. Enchows that the result can be extended

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<v Speaker 1>to the third order of small quantities. These were the

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<v Speaker 1>memoirs which led to Lagrange's famous memoir of eighteen oh eight.

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<v Speaker 1>Poissan also published a paper in eighteen twenty one on

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<v Speaker 1>the libration of the Moon, and another in eighteen twenty

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<v Speaker 1>seven on the motion of the Earth about its center

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<v Speaker 1>of gravity. His most important memoirs and the theory of

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<v Speaker 1>attraction are one in eighteen twenty nine on the attraction

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<v Speaker 1>of spheroids, and another in eighteen thirty five on the

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<v Speaker 1>attraction of a homogeneous ellipsoid. The substitution of the correct

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<v Speaker 1>equation involving the potential, namely grad squared v equals negative

233
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<v Speaker 1>four pi row for Laplace's form of it, Pi squared

234
00:16:20.639 --> 00:16:24.039
<v Speaker 1>v equals zero was first published in eighteen thirteen in

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<v Speaker 1>De Bouditaine des science of the society Phiromatique. Lastly, I

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<v Speaker 1>may mention his memoir in eighteen twenty five on the

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<v Speaker 1>theory of waves. Empeire Andre Marie Ampere was born at

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<v Speaker 1>Leon in January twenty second, seventeen seventy five, and died

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<v Speaker 1>at Marseilles on June tenth, eighteen thirty six. He was

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<v Speaker 1>widely read in all branches of learning, and lectured and

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<v Speaker 1>wrote on many of them. But after the year eighteen

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<v Speaker 1>o nine, when he was made professor of analysis at

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<v Speaker 1>the Polytechnic School in Paris, he confined himself almost entirely

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<v Speaker 1>to mathematics and science. His papers on the connection between

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00:17:07.480 --> 00:17:12.480
<v Speaker 1>electricity and magnetism were written in eighteen twenty. According to

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00:17:12.519 --> 00:17:17.000
<v Speaker 1>his theory propounded in eighteen twenty six, a molecule of

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00:17:17.079 --> 00:17:20.799
<v Speaker 1>matter which can be magnetized is traversed by a cloud

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<v Speaker 1>of electric current, and a magnetization is produced by any

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<v Speaker 1>cause which makes the direction of these currents in the

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00:17:29.079 --> 00:17:35.319
<v Speaker 1>different molecules of the body approach parallelism. Fresnel Augustin Jean

251
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<v Speaker 1>Fresnel born at Broglie on May tenth, seventeen eighty eight

252
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<v Speaker 1>and died at Verderey on July fourteenth, eighteen twenty seven.

253
00:17:44.519 --> 00:17:47.759
<v Speaker 1>Was a civil engineer by profession, but he devoted his

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<v Speaker 1>leisure to the study of physical optics. The undulatory theory

255
00:17:52.359 --> 00:17:55.440
<v Speaker 1>of light, which huck Reugens and Euler had supported on

256
00:17:55.559 --> 00:17:59.240
<v Speaker 1>a priori grounds, had been based on experiment by the

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00:17:59.319 --> 00:18:05.920
<v Speaker 1>researches of Fresnel deduced the mathematical consequences of these experiments

258
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<v Speaker 1>and explained the phenomenon of the interference of both ordinary

259
00:18:10.200 --> 00:18:16.759
<v Speaker 1>and polarized light. Billout Fresnel's friend and contemporary, Jean Baptiste Biot,

260
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<v Speaker 1>who was born at Paris on April twenty first, seventeen

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<v Speaker 1>seventy four and died there in eighteen sixty two, requires

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<v Speaker 1>a word or two in passing. Most of his mathematical

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00:18:27.920 --> 00:18:31.319
<v Speaker 1>work was in connection with the subject of optics, and

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00:18:31.440 --> 00:18:35.759
<v Speaker 1>especially with the polarization of light. His systematic works were

265
00:18:35.839 --> 00:18:39.279
<v Speaker 1>produced within the years eighteen o five. In eighteen seventeen,

266
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<v Speaker 1>a selection of his more valuable memoirs was published in

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<v Speaker 1>Paris in eighteen fifty eight. Arago Francois Jean Dominique Arago

268
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<v Speaker 1>was born at Estangel in the Pyrenees on February twenty

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<v Speaker 1>sixth seventeen eighty six and died in Paris on October second,

270
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<v Speaker 1>eighteen fifty three. He was educated at the Polytechnic School, Paris,

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<v Speaker 1>and we gather from his autobiography that, however distinguished were

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<v Speaker 1>the professors of that institution, they were remarkably incapable of

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<v Speaker 1>imparting their knowledge or maintaining discipline. In eighteen o four

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<v Speaker 1>he was made secretary to the Observatory, and then from

275
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<v Speaker 1>eighteen o six to eighteen o nine he was engaged

276
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<v Speaker 1>in measuring a meridian arc in order to determine the

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<v Speaker 1>exact length of a meter. He was then made one

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<v Speaker 1>of the astronomers at Paris, given a residence there, and

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<v Speaker 1>made a professor at the Polytechnic School, where he enjoyed

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<v Speaker 1>a marked success as a lecturer. He subsequently gave popular

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<v Speaker 1>lectures on astronomy, which were both lucid and accurate, a

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<v Speaker 1>combination of qualities which was rarer than now. He reorganized

283
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<v Speaker 1>the National Observatory, the management of which had long been inefficient.

284
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<v Speaker 1>But in doing this he shewed himself dictatorial and passionate,

285
00:19:59.160 --> 00:20:01.960
<v Speaker 1>and the same defaul efects of character revealed themselves in

286
00:20:02.039 --> 00:20:05.519
<v Speaker 1>many of the events of his life. He remained to

287
00:20:05.559 --> 00:20:09.440
<v Speaker 1>the end a consistent Republican, and after the Coup d'ettas

288
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<v Speaker 1>of eighteen fifty two, though half blind and dying, he

289
00:20:13.960 --> 00:20:17.359
<v Speaker 1>resigned his post as an astronomer rather than take the

290
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<v Speaker 1>oath of allegiance. It is to the credit of Napoleon

291
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<v Speaker 1>the Third that he gave directions that the old man

292
00:20:24.799 --> 00:20:27.559
<v Speaker 1>should be in no way disturbed, and that he should

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00:20:27.559 --> 00:20:29.400
<v Speaker 1>be left free to say and do what he liked.

294
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<v Speaker 1>His earliest physical researches were on the pressure of steam

295
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<v Speaker 1>at different temperatures and the velocity of sound eighteen eighteen

296
00:20:39.680 --> 00:20:44.440
<v Speaker 1>to eighteen twenty two. His magnetic observations mostly took place

297
00:20:44.799 --> 00:20:49.200
<v Speaker 1>from eighteen twenty three to eighteen twenty six. He discovered

298
00:20:49.319 --> 00:20:53.559
<v Speaker 1>what had been called rotary magnetism and the fact that

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00:20:53.640 --> 00:20:58.039
<v Speaker 1>most bodies could be magnetized. These discoveries were completed and

300
00:20:58.160 --> 00:21:03.519
<v Speaker 1>explained by Faraday. He warmly supported Fresnel's optical theories, and

301
00:21:03.640 --> 00:21:08.319
<v Speaker 1>the two philosophers conducted together those experiments on the polarization

302
00:21:08.400 --> 00:21:11.920
<v Speaker 1>of light, which led to the interference that the vibrations

303
00:21:11.960 --> 00:21:15.960
<v Speaker 1>of the luminiferous ether were transverse to the direction of motion,

304
00:21:16.799 --> 00:21:21.240
<v Speaker 1>and that the polarization consisted in a resolution of rectilinear

305
00:21:21.319 --> 00:21:25.920
<v Speaker 1>motion into components at right angles to each other. The

306
00:21:25.960 --> 00:21:30.799
<v Speaker 1>subsequent invention of the polariscope and the discovery of rotatory

307
00:21:30.839 --> 00:21:35.920
<v Speaker 1>polarization are due to Arago. The general idea of the

308
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<v Speaker 1>experimental determination of the velocity of light in the manner

309
00:21:39.519 --> 00:21:44.119
<v Speaker 1>subsequently affected by Faisot and Foucot, was suggested by him

310
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<v Speaker 1>in eighteen thirty eight, but his failing eyesight prevented his

311
00:21:48.720 --> 00:21:53.119
<v Speaker 1>arranging the details or making the experiments. It will be

312
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<v Speaker 1>noticed that some of the last members of the French

313
00:21:56.680 --> 00:22:01.559
<v Speaker 1>school were alive at a comparatively recent date, but nearly

314
00:22:01.640 --> 00:22:05.079
<v Speaker 1>all mathematical work was done before the year eighteen thirty.

315
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<v Speaker 1>They are the direct successors of the French writers who

316
00:22:09.240 --> 00:22:13.319
<v Speaker 1>flourished at the commencement of this century, and seem to

317
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<v Speaker 1>have been out of touch with the great German mathematicians

318
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<v Speaker 1>of the early part of it, on whose researches much

319
00:22:19.640 --> 00:22:22.759
<v Speaker 1>of the best work of this century is based. They

320
00:22:22.799 --> 00:22:25.240
<v Speaker 1>are thus placed here, though their writings are in some

321
00:22:25.440 --> 00:22:28.160
<v Speaker 1>cases of a later date than those of gauss Abel,

322
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<v Speaker 1>Jacobi and other mathematicians of recent times. The introduction of

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00:22:34.880 --> 00:22:40.519
<v Speaker 1>analysis into England, the complete isolation of the English school

324
00:22:40.559 --> 00:22:44.079
<v Speaker 1>and its devotion to geometrical methods are the most marked

325
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<v Speaker 1>features in its history during the latter half of the

326
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<v Speaker 1>eighteenth century, and the absence of any considerable and valuable

327
00:22:51.039 --> 00:22:56.160
<v Speaker 1>contributions to the advancement of mathematical science was a natural consequence.

328
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<v Speaker 1>One result of this was that the energy of the

329
00:23:00.279 --> 00:23:04.400
<v Speaker 1>englishmen of science was largely devoted to practical physics and

330
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<v Speaker 1>practical astronomy, which were in consequence studied in Britain, perhaps

331
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<v Speaker 1>more than elsewhere. Almost the only English mathematician at the

332
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<v Speaker 1>beginning of this century who used analytical methods and whose

333
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<v Speaker 1>work requires mentioned here is Ivory, to whom the celebrated

334
00:23:21.599 --> 00:23:25.920
<v Speaker 1>theorem of attractions is due. James Ivory was born in

335
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<v Speaker 1>Dundee in seventeen sixty five and died at Douglastown on

336
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<v Speaker 1>September twenty first, eighteen forty five. After graduating at Saint Andrews,

337
00:23:35.440 --> 00:23:38.559
<v Speaker 1>he became the managing partner in a flax spinning company

338
00:23:38.640 --> 00:23:42.319
<v Speaker 1>in Forfardshire, but continued to devote most of his leisure

339
00:23:42.400 --> 00:23:46.319
<v Speaker 1>to mathematics. In eighteen o four he was made professor

340
00:23:46.359 --> 00:23:49.640
<v Speaker 1>at the Royal Military College at Marlow, which has now

341
00:23:49.680 --> 00:23:55.680
<v Speaker 1>moved to Sandhurst. He contributed numerous papers to the Philosophical Transactions,

342
00:23:55.759 --> 00:23:59.480
<v Speaker 1>the most remarkable being those on attractions. In one of these,

343
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<v Speaker 1>in eighteen he shewed how the attraction of a homogeneous

344
00:24:03.079 --> 00:24:06.720
<v Speaker 1>ellipsoid on an external point is a multiple of that

345
00:24:06.839 --> 00:24:10.559
<v Speaker 1>of another ellipsoid on an internal point, the latter can

346
00:24:10.640 --> 00:24:15.319
<v Speaker 1>be easily obtained. He criticized Laplace's solution of the method

347
00:24:15.359 --> 00:24:19.519
<v Speaker 1>of Lee squares with unnecessary bitterness and in terms which

348
00:24:19.559 --> 00:24:24.319
<v Speaker 1>proved his incompetence to understand it. The Cambridge Analytical school.

349
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<v Speaker 1>Toward the close of the last century, the more thoughtful

350
00:24:27.599 --> 00:24:31.039
<v Speaker 1>members of the Cambridge School of Mathematics began to recognize

351
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<v Speaker 1>that their isolation from the continental contemporaries was a serious evil.

352
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<v Speaker 1>The earliest attempt in England to explain the notation and

353
00:24:40.279 --> 00:24:43.519
<v Speaker 1>methods of the calculus as used on the continent was

354
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<v Speaker 1>due to Woodhouse, who stands out as the apostle of

355
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<v Speaker 1>the new movement. It is doubtful if he could have

356
00:24:50.279 --> 00:24:53.799
<v Speaker 1>brought the analytical methods into vogue by himself, but his

357
00:24:53.960 --> 00:24:59.279
<v Speaker 1>views were enthusiastically adopted by three undergraduates, Babbage, Peacock and Herschel,

358
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<v Speaker 1>who he succeeded in carrying out reforms that he had

359
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<v Speaker 1>suggested in a book which will fall into the hands

360
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<v Speaker 1>of few but English readers. I may be pardoned for

361
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<v Speaker 1>making space for a few remarks on these four mathematicians.

362
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<v Speaker 1>The original stimulus came from French sources, and I therefore

363
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<v Speaker 1>placed these remarks at the close of my account of

364
00:25:20.160 --> 00:25:23.519
<v Speaker 1>the French school. But I should add that the English

365
00:25:23.559 --> 00:25:27.119
<v Speaker 1>mathematicians of this century at once struck out a line

366
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<v Speaker 1>independent of their French contemporaries. Woodhouse Robert Woodhouse was born

367
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<v Speaker 1>at Norwich on April twenty eighth, seventeen seventy three. Was

368
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<v Speaker 1>educated at Caius College, Cambridge, of which society he was

369
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<v Speaker 1>subsequently a fellow, was Plumian Professor in the university, and

370
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<v Speaker 1>continued to live at Cambridge till his death on December

371
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<v Speaker 1>twenty third, eighteen twenty seven. His earliest work, entitled The

372
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<v Speaker 1>Principles of Analytical Calculation, was published at Cambridge in An

373
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<v Speaker 1>eighteen o three. In this he explained the differential notation

374
00:26:05.039 --> 00:26:09.079
<v Speaker 1>and strongly pressed the employment of it, but he severely

375
00:26:09.119 --> 00:26:13.960
<v Speaker 1>criticized the methods used by Continental writers and their constant

376
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<v Speaker 1>assumption of non evident principles. This was followed in eighteen

377
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<v Speaker 1>o nine by a trigonometry Plain and Spherical, and in

378
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<v Speaker 1>eighteen ten by historical treatise on the Calculus of variations

379
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<v Speaker 1>and isoparametrical problems. He next produced an Astronomy, the first

380
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<v Speaker 1>volume usually bound in two on practical and Descriptive Astronomy,

381
00:26:38.359 --> 00:26:41.920
<v Speaker 1>being issued in eighteen twelve, the second volume, containing an

382
00:26:41.960 --> 00:26:45.759
<v Speaker 1>account of the treatment of physical astronomy by Laplace and

383
00:26:45.920 --> 00:26:50.880
<v Speaker 1>other Continental writers, being issued in eighteen eighteen. All these

384
00:26:50.920 --> 00:26:55.519
<v Speaker 1>works deal critically with the scientific foundation of the subjects considered,

385
00:26:55.839 --> 00:27:00.319
<v Speaker 1>a point which is not unfrequently neglected in modern textbook boks.

386
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<v Speaker 1>A man like Woodhouse, of scrupulous honor, universally respected, a

387
00:27:07.680 --> 00:27:11.480
<v Speaker 1>trained logician, and with a caustic wit, was well fitted

388
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<v Speaker 1>to introduce a new system. And the fact that when

389
00:27:14.640 --> 00:27:18.680
<v Speaker 1>he first called attention to the Continental analysis, he exposed

390
00:27:18.720 --> 00:27:22.319
<v Speaker 1>the unsoundness of some of the usual methods of establishing it.

391
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<v Speaker 1>More like an opponent than a partisan, and was politic

392
00:27:26.839 --> 00:27:30.799
<v Speaker 1>as it was honest. Woodhouse did not exercise much influence

393
00:27:30.799 --> 00:27:34.759
<v Speaker 1>on the majority of his contemporaries, and the movement might

394
00:27:34.759 --> 00:27:37.319
<v Speaker 1>have died away for the time being had it not

395
00:27:37.400 --> 00:27:42.359
<v Speaker 1>been for the advocacy of Peacock, Herschel and Babbage, who

396
00:27:42.400 --> 00:27:46.759
<v Speaker 1>formed an analytical Society with the object of advocating the

397
00:27:46.880 --> 00:27:50.759
<v Speaker 1>general use in the University of analytical methods and of

398
00:27:50.799 --> 00:27:57.240
<v Speaker 1>the differential notation. Peacock George Peacock, who was the most

399
00:27:57.240 --> 00:27:59.839
<v Speaker 1>influential of the early members of the New School, was

400
00:28:00.000 --> 00:28:04.960
<v Speaker 1>born at Denton on April ninth, seventeen ninety one. He

401
00:28:05.079 --> 00:28:09.440
<v Speaker 1>was educated at Trinity College, Cambridge, of which society he

402
00:28:09.559 --> 00:28:13.400
<v Speaker 1>was subsequently a fellow and tutor. The establishment of the

403
00:28:13.519 --> 00:28:16.720
<v Speaker 1>University Observatory was mainly due to his efforts, and in

404
00:28:16.799 --> 00:28:20.359
<v Speaker 1>eighteen thirty six he was appointed to the Loundean Professorship

405
00:28:20.440 --> 00:28:24.279
<v Speaker 1>of Astronomy and Geometry. In eighteen thirty nine he was

406
00:28:24.359 --> 00:28:28.200
<v Speaker 1>made Dean of Eli and resided there until his death

407
00:28:28.200 --> 00:28:32.680
<v Speaker 1>in November eighth, eighteen fifty eight. Although Peacock's influence on

408
00:28:32.759 --> 00:28:38.240
<v Speaker 1>English mathematicians was considerable, he has left but few memorials

409
00:28:38.279 --> 00:28:41.720
<v Speaker 1>to his work. But I may note that his Report

410
00:28:41.799 --> 00:28:45.759
<v Speaker 1>on Recent Progress and Analysis eighteen thirty three commenced those

411
00:28:45.839 --> 00:28:49.920
<v Speaker 1>valuable summaries of scientific progress which enriched many of the

412
00:28:49.960 --> 00:28:57.640
<v Speaker 1>annual volumes of the transactions of the British Association Babbage.

413
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<v Speaker 1>Another important member of the Analyticalsis Society was Charles Babbage,

414
00:29:02.240 --> 00:29:06.720
<v Speaker 1>who was born at Totna's in December twenty sixth, seventeen

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<v Speaker 1>ninety two. He entered Trinity College, Cambridge in eighteen ten,

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<v Speaker 1>subsequently became Lucasian Professor in the university, and died in

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<v Speaker 1>London on October eighteenth, eighteen seventy one. It was he

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<v Speaker 1>who gave the name to the Analytical Society, which he

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<v Speaker 1>stated was formed to advocate the principles of pure Deism

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<v Speaker 1>as opposed to the dottage of the university. In eighteen

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<v Speaker 1>twenty the Astronomical Society was founded mainly through his efforts,

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<v Speaker 1>and at a later time eighteen thirty to eighteen thirty

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<v Speaker 1>two he took a prominent part in the foundation of

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<v Speaker 1>the British Association. He will be remembered for his mathematical

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<v Speaker 1>memoirs on the calculus of functions, and in the invention

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<v Speaker 1>of analytical machines which could not only perform ordinary processes

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<v Speaker 1>of a ru arithmetic, but could tabulate the values of

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<v Speaker 1>any functions and print the results. Herschel the third of

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<v Speaker 1>those who helped bring analytical methods into general use in England.

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<v Speaker 1>Was the son of Sir William Herschel seventeen thirty eight

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<v Speaker 1>to eighteen twenty two, the most illustrious astronomer of the

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<v Speaker 1>latter half of the last century, and the creator, it

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<v Speaker 1>may be fairly said, of stellar astronomy. Sir John Frederick

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<v Speaker 1>William Herschel was born on March seventh, seventeen ninety two

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<v Speaker 1>and educated at Saint John's College, Cambridge, and died on

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<v Speaker 1>May eleventh, eighteen seventy one. His earliest original work was

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<v Speaker 1>a paper on Coates's theorem, and it was followed by

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<v Speaker 1>others on mathematical analysis, but his desire to complete his

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<v Speaker 1>father's work led ultimately to his taking up astronomy. His

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<v Speaker 1>papers on light and astronomy contain a clear exposition of

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<v Speaker 1>the principles which underline the mathematical treatment of those subjects.

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<v Speaker 1>In eighteen thirteen, the Analytical Society published a volume of memoirs,

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<v Speaker 1>of which the preface and the first paper on continued

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<v Speaker 1>products are due to Babbage and the Three years later

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<v Speaker 1>they issued a translation of Lacrois tret des elementaire to

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<v Speaker 1>calcur differentier et du calcur integral in eighteen seventeen and

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<v Speaker 1>again in eighteen nineteen. The differential notation was used in

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<v Speaker 1>the university examinations, and after eighteen twenty its use was

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<v Speaker 1>well established. The Analytical Society followed up this rapid victory

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<v Speaker 1>by the issue in eighteen twenty of two volumes of

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<v Speaker 1>examples illustrative of the new method, one by Peacock on

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<v Speaker 1>the differential and integral calculus and the other by Herschel

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<v Speaker 1>on the calculus of finite differences. Since then, English works

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<v Speaker 1>on the infinitesimal calculus have a bet have abandoned the

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<v Speaker 1>exclusive use of the fluctional notation. It should be noticed

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<v Speaker 1>in passing that Lagrange and Laplace, like the majority of

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<v Speaker 1>other modern writers, employ both the fluctional and the differential notation.

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<v Speaker 1>It was the exclusive adoption of the former that was

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<v Speaker 1>so hampering. Amongst those who materially assisted in extending the

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<v Speaker 1>use of the new analysis were William Wherwell seventeen ninety

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<v Speaker 1>four to eighteen sixty six and George Beidell Airy eighteen

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<v Speaker 1>o one to eighteen ninety two, both fellows at Trinity College, Cambridge.

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<v Speaker 1>The former issued in eighteen nineteen a work on Mechanics,

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<v Speaker 1>and the latter, who was a pupil of Peacock, published

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<v Speaker 1>in eighteen twenty six in his Tracts, in which the

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<v Speaker 1>new method was applied with great success to various physical problems.

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<v Speaker 1>The efforts of the society were supplemented by the rapid

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<v Speaker 1>publication of good texts books in which analysis was freely used.

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<v Speaker 1>The employment of analytical methods spread from Cambridge over the

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<v Speaker 1>rest of Britain, and by eighteen thirty those methods have

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<v Speaker 1>come into general use there end of section thirty two.

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<v Speaker 1>Recording by Paul King, Mississauga, Ontario, h d T, P

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<v Speaker 1>p J K dot scripts dot m I T dot

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<v Speaker 1>E d U forward slash p k J
