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During the 1970s, the Meteorological Office's numerical models of the global atmospheric circulation began to simulate the main features of the world's climate and its variations and show that the climatic consequence of increasing the carbon dioxide content of the atmosphere was global warming. The Office's previous predictions by simpler models of a general warming much accentuated in polar regions were confirmed, but further study with improved models and a more powerful computer would be required to assess these climatic effects and their likely economic and social impact with real confidence.
The causes and the economic and social consequences of climatic change were debated in the House of Lords on 30 November 1978. The opening speaker, Lord Tanlaw, asked the government whether there was cause for concern in the current increase in atmospheric carbon dioxide and apparent change in global weather patterns. He referred to an article by the Office's Director-General that had been published in Nature (1978, Vol. 276, pp. 327–328). In this, Dr Mason had suggested that a doubling of carbon dioxide would lead to an increase in global temperature of two or three degrees Celsius. Though this was a modest increase, Lord Tanlaw said, it “might well lead to increased food production by prolonging the growing season and, furthermore, produce considerable savings in energy consumption”. There might, though, be “unforeseen disadvantages”, such as adverse effects on agriculture in some parts of the world as a result of changes in rainfall patterns. The melting of glaciers might also cause sea level to rise and thus threaten coastal communities.
The first ‘flying machines’ were flimsy and the motions of the atmosphere capricious. Many an early aeroplane was damaged or wrecked when dashed to the ground by an unexpected gust of wind. The pioneers of aviation certainly needed meteorological assistance, and the French pilot Louis Paulhan did indeed gain some when, in April 1910, he won the prize of £10,000 offered by the Daily Mail for being the first to fly between London and Manchester in under twenty-four hours. The Meteorological Office made elaborate provision to keep him supplied with information about the prospective weather en route.
The Emergence of Aeronautics
The Prime Minister, Herbert Asquith, informed the House of Commons on 5 May 1909 that the Government wished to apply the “highest scientific talent” to problems of aerial navigation. He had appointed a special committee which would be chaired by Dr Glazebrook, Director of the NPL, and include among its members Dr Shaw, Director of the Office.
The Met Office is a well-respected and familiar British institution, whose weather forecasts people hear every day. News about its activities and advice are discussed at length in the media and in Parliament. It was founded in 1854 and still goes strong. Queen Victoria had personal weather forecasts from Admiral FitzRoy, the first director, for her three-mile voyage across the Solent to the Isle of Wight. It is not an exaggeration to say that the Office has played an important part in the history of the United Kingdom and of many other countries over this period, in both peace and war. Although it is an institution based on the application of science and technology, its outstanding staff have in fact originated some of the key developments of meteorological science and technology, a tradition that continues today.
This book had its origins in the PhD of the late Dr Jim Burton, a forecaster in the Leeds Weather Centre, who was encouraged by Sir John Houghton, then Director-General of the Met Office. His predecessor, Sir John Mason, helped the project. The necessary financial ingenuity to arrange funding for research into the history of the Office was provided by Martyn Bittlestone, our finance director, when the Office became a Trading Fund in 1996. The Chief Scientist, Professor Julia Slingo, has helped recently with her insights into developments up to 2010. I am very grateful to Malcolm Walker, formerly of Cardiff University, for accepting the invitation not only to write the book but also to listen tactfully to all the inputs from meteorologists and commentators on the text. Stan Cornford's detailed study in 1994 of the Met Office involvement in the D-Day forecast was also a significant contribution.
Some of the most distinguished scientists in the land were members of the Meteorological Council, but to little effect. As a scientific institution, the Meteorological Office was moribund in the 1890s. A scientist with vision was required.
Changes in membership were rare, and those that did occur were forced. Sir John Lefroy deputized for Richard Strachey from April 1878 to April 1879 (whilst Strachey was in India, advising the India Meteorological Department). Professor Smith died in February 1883, and the vacancy that resulted from Strachey succeeding Smith as Chairman was filled by the Radcliffe Observer, Edward Stone. William Wharton succeeded Frederick Evans as Hydrographer in July 1884, and George Darwin joined the Council in February 1885, when Warren De La Rue resigned because of failing health. George Stokes resigned in November 1887, when elected Member of Parliament for the University of Cambridge, and his place on the Council went to Alexander Buchan, to represent the Scottish Meteorological Society. Thereafter, there were no more changes in membership for nearly ten years.
To mark the fiftieth anniversary of the Office, Laura FitzRoy presented a portrait of her father. This was reported at the meeting of the Meteorological Council on 19 October 1904, but the anniversary otherwise passed largely unnoticed. FitzRoy's era had long since passed. However, another reason for the passing of the anniversary with so little attention paid to it could have been preoccupation with the report of an inquiry published in 1904.
Yet Another Inquiry
The impending closure of the Ben Nevis and Fort William observatories was the subject of questions asked in the House of Commons in 1902. For example, John Dewar asked the First Lord of the Treasury on 28 July whether the Government, in giving an annual grant of £15,300 to the Office, would make it a condition that these observatories “be maintained in a state of efficiency, or consider the advisability of making an additional contribution to the Meteorological Council towards the expense of properly maintaining them”. The Prime Minister, Arthur Balfour, replied, saying that he had been advised “it would not be desirable to impose conditions on the Meteorological Council or to inquire into this or that particular observatory”. He was not prepared, he said, to answer the part of the question relating to an additional contribution.
Sir George Simpson retired on 2 September 1938, his sixtieth birthday. Who would succeed him? This matter had been addressed as early as 21 February 1936, in an internal minute from J B Abraham, an Assistant Secretary in the Air Ministry, to J A Webster, a Principal Assistant Secretary.
Abraham had ruled out Lempfert and Whipple on grounds of age and ruled out Gold, too, but not on grounds of age, even though he would have been 57 when Simpson retired. Rather, there were misgivings about him. Abraham doubted he had “the administrative ability requisite in the Director of a big department” and commented that his temperament was “rather difficult”. Abraham also ruled out Corless, Entwistle, Goldie, J S Dines and E G Bilham, the five in the Principal Technical Officer grade. His conclusion was that none had shown the all-round scientific and administrative ability a Director needed. Simpson's successor would need to be someone not currently a member of the Office's staff. In Abraham's view, the field of selection was “rather restricted”. Brunt might be a possibility but appeared to “lack the personality and all-round ability which was desirable”. Perhaps the most suitable successor was Watson Watt. He was, Abraham said, “a scientist of great ability and exceptional energy”.
Sir Napier Shaw died on 23 March 1945, aged 91. In his lifetime, meteorology had been transformed, partly through his scientific insight, inspiration and leadership, but also through technological developments such as wireless telegraphy, aircraft, the radiosonde and radar. He had given the UK a leading position in international meteorology and laid the foundations which had been built upon in peacetime and wartime to form the institution the Meteorological Office had become by 1945, a scientific and technological body of national and international importance.
Further Reorganization of the Meteorological Office
Hardly had the war ended when there came yet another reorganization of the Office, this one the outcome of an inquiry into the constitution of the Scientific Civil Service. The inquiry had been carried out during the war by a committee chaired by Sir Alan Barlow, a Treasury under-secretary, and its recommendations had been presented to Parliament in September 1945 in a White Paper (Cmd. 6679). The Office was reorganized on the lines the Barlow Committee recommended. Out went the grades that had been introduced in the 1930s in response to the report of the Carpenter Committee (see Chapter 9). In came the grades of Scientific Officer, Experimental Officer and Scientific Assistant, and with them came revised scales of pay.
Charles Daubeny (1795–1867) first published Active and Extinct Volcanos in 1826. This reissue is of the second, augmented edition of 1848, which the author explains was significantly updated in the light of the work of Charles Darwin. Part I contains geological descriptions of most of the world's known volcanos, arranged by region, many of them based on Daubeny's own observations. Part II contains descriptions of earthquake-prone regions, thermal springs, and thermal waters. In Part III Daubeny introduces his influential theory of the causes of volcanic action, proposing that it results from contact between water and metals beneath the earth's surface. He also discusses the factors that give volcanos particular characteristics, and the impact of volcanos on their environments. This pioneering work of Victorian geology provided the scientific community with some of the first descriptions and data sets on previously unstudied volcanic regions, and is still referred to today.
First published in 1894, this biography details the life of renowned geologist William Buckland (1784–1856) who, along with Sedgwick and Lyell, was one of the pioneers of modern geological inquiry. While he is better known for attempting to correlate his geological findings with the Old Testament, Buckland's studies paved the way for Darwin's development of evolutionary theory. In the course of his illustrious career, Buckland was a Canon of Christ Church, was twice appointed President of the Geological Society, served as the first President of the British Association, and became Dean of Westminster. Penned by Buckland's daughter almost forty years after his death, The Life and Correspondence provides a more personal insight into Buckland's scientific endeavours. Gordon's biography is complemented by several illustrations, and the appendices include an extensive list of positions held by Buckland and his membership of learned societies, and a complete index of his publications.
This paper argues that the 1953 double-helix solution to the problem of DNA structure was understood, at the time, as a blow within a fiercely fought dispute over the material nature of life. The paper examines the debates, between those for whom life was a purely material phenomenon and religious people for whom it had a spiritual significance, that were waged from the aftermath of the First World War to the 1960s. It looks at the developing arguments of early promoters of molecular biology, including J.D. Bernal, his pupil Max Perutz and his pupil Francis Crick, on the one side, and of the so-called ‘Inkling’ cluster of writers including C.S. Lewis and J.R.R. Tolkien, on the other. This debate was conducted through polemical works, journalism, and science fiction and through the Festival of Britain and can be followed through the commentary of Jacob Bronowski. The paper concludes with the model of the double helix now at the Science Museum, which can be considered an archaeological relic of a battle in a war which is still being fought.
UK defence R & D played a leading role in the development of gallium arsenide and other III–V semiconductor materials. Often touted as the semiconductor of the future because of its potential for high-speed computing, gallium arsenide had unique properties compared to silicon that made it attractive for military applications. Some consumer applications were also developed, and these eventually became significant with its use in mobile phone handsets in the mid-1990s. However, despite the apparent advantage of close links to the defence establishments and early access to expertise in III–V technologies, UK companies had limited success in these civil markets, preferring instead to focus on defence procurement.
It has been traditionally held that the idea of a prime matter of metals was abandoned in the eighteenth century, especially after the failure of Hermann Boerhaave to find it in mercury. However, documents tell a different story: the search for the metalliferous principle, in the form of an odd substance known as Gur, Guhr, Ghur or Bur, was very much alive in the 1700s. This was a project that involved Boerhaave himself, as is shown by his correspondence with J.B. Bassand. The first mention of this strange material appears in Sarepta, a collection of sermons by the sixteenth-century Bohemian preacher Johannes Mathesius, sometimes mentioned in the specialized literature but rarely studied. This paper discusses the various conceptions of this material held as the prime matter of metals, from Mathesius to the eighteenth century, involving reputed authors such as John Webster, Jan B. van Helmont, Georg E. Stahl and Boerhaave.
Historians have given much attention to museums and exhibitions as sites for the production and communication of knowledge in the nineteenth and early twentieth centuries. But few studies have analysed how the activity and participation of visitors was designed and promoted at such locations. Using Francis Galton's Anthropometric Laboratory at the International Health Exhibition in London 1884 as the empirical focal point, this paper explores a new mode of involving exhibition audiences in the late nineteenth century. Its particular form of address is characterized by an ambition to transform the visitors' self-understanding by engaging them with various techniques of scientific observation and representation of social issues. By analysing the didactics of this particular project, I argue that the observational ideal of ‘mechanical objectivity’ and associated modes of representation in this instance became an integrated part of a political vision of self-observation and self-reformation. Thus the exhibit and related projects by Galton not only underpinned a theoretical lesson, but also were part of an effort to extend a complex set of practices among the general public.
In March 1742, British naval officer John Byron witnessed a murder on the western coast of South America. Both Charles Darwin and Robert FitzRoy seized upon Byron's story a century later, and it continues to play an important role in Darwin scholarship today. This essay investigates the veracity of the murder, its appropriation by various authors, and its false association with the Yahgan people encountered during the second voyage of the Beagle (1831–1836). Darwin's use of the story is examined in multiple contexts, focusing on his relationship with the history of European expansion and cross-cultural interaction and related assumptions about slavery and race. The continuing fascination with Byron's story highlights the key role of historical memory in the development and interpretation of evolutionary theory.
Georges-Louis Leclerc, Comte de Buffon (1707–88), was a French mathematician who was considered one of the leading naturalists of the Enlightenment. An acquaintance of Voltaire and other intellectuals, he worked as Keeper at the Jardin du Roi from 1739, and this inspired him to research and publish a vast encyclopaedia and survey of natural history, the ground-breaking Histoire Naturelle, which he published in forty-four volumes between 1749 and 1804. These volumes, first published between 1770 and 1783 and translated into English in 1793, contain Buffon's survey and descriptions of birds from the Histoire Naturelle. Based on recorded observations of birds both in France and in other countries, these volumes provide detailed descriptions of various bird species, their habitats and behaviours and were the first publications to present a comprehensive account of eighteenth-century ornithology. Volume 2 covers wild and domestic fowl and pigeons.
Alfred Russel Wallace (1823–1913) was a British naturalist, explorer, geographer and biologist, best remembered as the co-discoverer, with Darwin, of natural selection. His extensive fieldwork and advocacy of the theory of evolution led to him being considered one of the nineteenth century's foremost biologists. He was later moved by a variety of personal experiences to examine the concept of spirituality, but his exploration into the potential for compatibility between spiritualism and natural selection alienated him from the scientific community. He was also a social activist, highly critical of unjust social and economic systems in nineteenth-century Britain, and one of the first prominent scientists to express concern over the environmental impact of human activity. This autobiography was first published in 1905. Volume 1 covers his childhood, his early social activism, and his expeditions to the Amazon and the Malay archipelago, which established his reputation.
Turbulence is widely recognized as one of the outstanding problems of the physical sciences, but it still remains only partially understood despite having attracted the sustained efforts of many leading scientists for well over a century. In A Voyage Through Turbulence we are transported through a crucial period of the history of the subject via biographies of twelve of its great personalities, starting with Osborne Reynolds and his pioneering work of the 1880s. This book will provide absorbing reading for every scientist, mathematician and engineer interested in the history and culture of turbulence, as background to the intense challenges that this universal phenomenon still presents.