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Re: Basics of computing sunrise/sunset
From: Douglas Denny
Date: 2009 Jun 18, 11:22 -0700
From: Douglas Denny
Date: 2009 Jun 18, 11:22 -0700
Perhaps a longer account from the RS Crookes report might be worthwhile for interest's sake:- Douglas Denny. Chichester. England. =========== Quote:- The work of Crookes's group Given the uncomfortably hot conditions in which glassblowers worked, it was a reasonable assumption that any damage done to their eyes was due to infrared radiation. Burch began work immediately on an empirical study of whether protective glass screens would allow workers to see what they were doing while shielding them from damaging glare. Aided by his demonstrator, T. G. Malpas, at the Physiological Laboratory in Oxford, Burch used Nernst filaments as sources because of their high temperatures and steadiness of light. These lamps were bought with the Committee's grant. The two men gathered much useful data on the percentages of light transmitted through various tinted glasses and also showed that transmission of radiation was dampened when thin coats of metallic film were applied to glasses. Unfortunately, such films caused blurring of images, which would have been dangerous for any bottle blower in factory conditions. The application of gauze screens in front of blue glass screens was also effective, but again raised doubts as to whether optical definition would be compromised.14 Meanwhile, Crookes undertook long-term research into how the addition of metal oxides to glass recipes might produce a glass that would reflect infrared light produced in the glare of white-hot furnaces. Made into safety spectacles, such a glass would prevent, or at least reduce, damage to the eyes of workmen fashioning molten glass. Crookes's investigations were partly made at his home laboratory in Notting Hill with his assistant James Gardiner (who had replaced Gimingham in 1881), and partly at the 230-year-old Whitefriars glassworks of Harry Powell, an Oxford-educated chemist. The firm of James Powell & Sons had been distinguished for its manufacture of coloured (stained) glasses since 1851.15 Crookes also took photographs of the spectra of molten glass while visiting the Nuttall bottle works in St Helens, the owner being particularly keen to save his workforce's eyesight. Although Nuttall had the opening in a glass furnace bricked up, leaving a small hole for the spectroscope, the fiercely hot conditions cannot have been pleasant for an 80-year-old man, and it was Gardiner who undertook much of the on-site measurements. Several of the exposures taken lasted three-quarters of an hour. Crookes rapidly determined that any worker exposed to the brilliant light from the furnace for three hours would receive a massive dose of infrared radiation, and he recalled how the Palm House at Kew Gardens used pale-green glass opaque to the infrared. He believed that ?spectacles or screens made of this glass might be of use in glassworks if the workmen would use them?.16 By 1909, however, Crookes became aware of French and German research showing that pathological changes to the eye lens were probably caused by ultraviolet radiation and that French glassmakers had succeeded in developing a coloured glass that dampened its transmission. This amber-coloured ?Euphos glass? rapidly entered the catalogues of spectacle manufacturers all over the world, the prescriptions being especially recommended for the goggles of sportsmen and drivers of automobiles. Crookes and Gardiner believed that this kind of tinted glass could be bettered if the absorption spectra of different types of glass were accurately determined. It was not until the summer of 1911 that Crookes was able to report to the Committee on successful formulations after appraising and comparing about 160 different combinations of metallic glass with white clear glass. In theory, he told the Committee, ?it should be possible to make a glass which would be opaque to the infrared and the ultraviolet, and my endeavours have been directed for some time towards that end, but hitherto I have not been successful?.17 Clearly, a compromise formulation would be necessary. Interestingly, he first tested the suitability of each metal ion by cutting a specimen of a pure metal into a thin plate 2 mm thick and using it as a radiometer vane to determine the relative order in which heat was cut off. Each metal was then tested spectroscopically to identify the limits of its ultraviolet spectrum, as well as its opacity (percentage of light rays transmitted) and colour in a tintometer. These tests had shown him that it was worth experimenting with glass mixtures containing small quantities of the oxides or salts of cerium, chromium, cobalt, copper, iron, lead, manganese, neodymium, nickel, praesodymium and uranium. Meanwhile, the government was badgering the Committee for results, but Crookes needed another two years' intermittent research and the inspiration of Faraday's glass researches before he was ready to go public.18 An interim report on the Committee's work and conclusions was sent to the Home Office in April 1911, after which the government gave a further ?100 towards a fuller investigation of the effects of light absorption on vision because it might have a bearing on the work of another government investigation of the lighting in factories and workshops, in which Parsons was centrally involved. The Committee decided, however, that it would need at least ?200 to accomplish this. To pump the government for the additional ?100 the Committee urged Crookes to write up his results quickly as proof that the research was offering value for money. Crookes's private report was subsequently formally presented to the Royal Society a month into his presidency in November 1913. The Home Office was clearly impressed and presented the Committee with the additional ?200 in January 1914. The paper announced a formulation that cut off 90% of heat radiation, was opaque to ultraviolet light, and was relatively free of colour so that objects remained clear to the eye. Crookes noted that, besides glassworkers, there would be an advantage in preparing such coloured or tinted glasses to prevent glare for people exposed to sunlight reflected off cliffs, snow, or even electric light."During the brilliant weather of the late summer [1911] I wore some of these spectacles with great comfort; they took off the whole glare of the sun on chalk cliffs, and did not appreciably alter the natural colours of objects. Lady Crookes, whose eyes are more sensitive to glare or strong light than are my own, wore them for several hours in the sun with great comfort.19" Crookes was not the first to prepare tinted lenses for leisure use, but here was the origin of scientifically formulated Crookes lenses or modern sunglasses.20 Crookes tested more than 300 tinted glasses for this swansong research project, each formulation receiving a serial number that entered the glass literature. The formulations he produced included ?specimens suitable for spectacles adapted to all requirements?from Eyes of Youth to Eyes of Age? (type 302). To cut off heat radiation he recommended Crookes Glass 246 (a sage-green glass containing ferrous oxalate with red tartar and wood charcoal) that eliminated 98% of the incident heat; for cutting out ultraviolet light the best glass was Crookes 158, containing cerium borate and ferric and chromic oxides; and for sunglasses the best choice was a pale blue Crookes 249 (Chance's Crookes Glass A1) containing cerium nitrate with a little ferric oxide and cobalt sulphate. All these glass formulations had been prepared with the cooperation of Chance Brothers at Birmingham, who exhibited samples at a Royal Society Conversazione in 1914,21 and by Powell's Whitefriars glassworks in London.22 The five-year research project also proved of considerable significance with the outbreak of war in August 1914. --~--~---------~--~----~------------~-------~--~----~ Navigation List archive: www.fer3.com/arc To post, email NavList@fer3.com To , email NavList-@fer3.com -~----------~----~----~----~------~----~------~--~---