From under the Nose

Author(s):  
Peter Wothers

This chapter looks at the elements in the final group of the periodic table—those elements known as the rare or noble gases. We shall see how their discovery in the atmosphere in the 1890s dates back to an observation first made by the meticulous Henry Cavendish over one hundred years earlier. This led to the unexpected discovery of an entire group of elements that needed to be added to the earliest periodic tables; and remarkably, one man was to dominate all these discoveries. One of Isaac Newton’s classic experiments was using a glass prism to split a beam of sunlight into a spectrum to show that white light is actually a mixture of all the colours of the rainbow. In 1802, William Hyde Wollaston (1766–1828), discoverer of the elements palladium and rhodium, modified the experiment by using a thin slit to admit the sunlight instead of the circular hole that Newton used. He subsequently discovered that the solar spectrum was not completely seamless, but actually contained a number of fine dark lines, now known as Fraunhofer lines. They get their name from Joseph Fraunhofer (1787–1826), who became the most skilled worker of glass and producer of lenses of the time. Using his highest-quality optical lenses, Fraunhofer observed that the solar spectrum had many dark lines; he mapped out over five hundred of these and designated the most distinct ones with the capitals letters A to H, with A and B being in the red region of the spectrum, and G and H in the violet. He used these as calibration lines in the development of better glasses for his optical instruments, and to demonstrate the superiority of his products compared with those of his competitors. The nature of the dark lines was not properly understood until the work of the German physicist Gustav Kirchhoff (1824–1997), who, in a beautiful collaboration with his colleague the chemist Robert Bunsen (1811–99), developed one of the most important analytical techniques still used in chemistry. It was with this technique that they discovered two new elements, and paved the way for others to discover many more.

Small ◽  
2019 ◽  
Vol 16 (1) ◽  
pp. 1905266 ◽  
Author(s):  
Guangqi Hu ◽  
Yuqiong Sun ◽  
Jianle Zhuang ◽  
Xuejie Zhang ◽  
Haoran Zhang ◽  
...  

2020 ◽  
Vol 59 (01) ◽  
pp. 1
Author(s):  
Xinran Zhang ◽  
Shuo Zhang ◽  
Guodong Wang ◽  
Yunyu Wang ◽  
Meng Liang ◽  
...  

1993 ◽  
Vol 141 ◽  
pp. 149-155 ◽  
Author(s):  
Guoxiang Ai

AbstractThe historical development of optical instruments for solar physics is outlined, from white light to unpolarized and polarized monochromatic light, to Stokes profiles and simultaneous fields of view, from points to lines, plane to cube. An evolutionary series and classificaton of instruments for the solar magnetic field is described. As a next step the 2-D real time polarizing spectrograph has been proposed. The planned instruments in China for measurements of solar magnetic and velocity fields are briefly introduced.


2016 ◽  
Vol 4 (21) ◽  
pp. 4728-4732 ◽  
Author(s):  
Muhammad Usman ◽  
Golam Haider ◽  
Shruti Mendiratta ◽  
Tzuoo-Tsair Luo ◽  
Yang-Fang Chen ◽  
...  

Natural white light emission from a Sr-based MOF with the highest sensitivity for the human eye and a good resemblance to the solar spectrum makes this compound an ideal choice for potential applications as a high performance lighting source.


In “Colour Photometry, Part III,” ‘Phil. Trans.,' 1892, and “On the Sensitiveness of the Retina to Light and Colour,” ‘Phil. Trans.,’ 1897, a discussion on the extinction of light by a “dark-adapted” eye is given. Since the latter date, a large number of experiments have been made by myself and others on the extinction of light when the retina as a whole has been stimulated by illumination of white or coloured light. In this communication the results obtained when the stimulation is by white light are described. In the two papers above referred to the apparatus used when the eye was dark-adapted is described, but for the observations made with an illuminated retina a modification had to be made. A description of one form, which answered as well as any other form, is given. BB is a box as in fig. 1. At the end of the box is cut a hole ¾ inch in diameter and against it, but inside, is placed a 4-inch disc of white matt paper, in the centre of which is cut a ½-inch circular hole. Behind the box is a second end AA separated from the first by a couple of inches. Opposite the aperture at the first end of the box is cut a circular aperture 1 inch in diameter, against which is placed a piece of doubly-ground white glass, and if necessary a second piece can be placed behind it. The ray of the spectrum from the colour-patch apparatus can be reflected from a mirror M on to the ground glasses at d . The 4-inch white disc is illuminated by the white reflected beam of the same apparatus (or by any other light) through an aperture CC cut in the side of the box. This beam partly goes through the aperture at the end of the box and falls on G, a blackened surface, and is completely hidden from the eye end E. At the side of CC a small metal disc can be placed, which casts a sharp black image on the white disc, as shown in fig. 2. This may be taken as a measure of the blackness to be matched when extinguishing the light from the colour.


1876 ◽  
Vol 24 (164-170) ◽  
pp. 186-189

Mv deae Sir,—I have the pleasure to send you, by Overland Parcel Post, for presentation to the Royal Society, two photographs on glass of the solar spectrum, showing the extreme red rays below A, obtained on a dry collodion plate prepared with bromide of silver stained with a blue and exposed to diffused daylight for a moment before being placed a the camera to receive the image of the spectrum. I also send another late, also a dry bromide plate, stained with the same blue dye, and prepared at the same time and in the same manner as the other plates, but not exposed to light and quite free from fog; and you will observe hat on this there is no trace of the reversed action in the red rays, and that the direct action only extends slightly below C. This power of the red rays of the spectrum to neutralize the action of white light on sensitive daguerreotype plates was frequently noticed by Sir J. Herschel, Draper, Fizeau, Claudet, and other daguerreotypists about thirty years ago, but, so far as I can ascertain, it has never been observed on collodion plates. As collodion has so many advantages over the daguerreotype, it seems probable that this new extension of an old principle may have an important practical application in spectroscopic photography, particularly for the mapping of a part of the spectrum in which eye-observations can only be made with difficulty and under favourable circumstances.


The object which the author has in view in this memoir is to place on record a number of insulated facts and observations respecting the relations both of white light, and of the differently refrangible rays, to various chemical agents which have offered themselves to his notice in the course of his photographic experiments, suggested by the announcement of M. Daguerre’s discovery. After recapitulating the heads of his paper on this subject, which was read to the Society on the 14th of March, 1839, he remarks, that one of the most important branches of the inquiry, in point of practical utility, is into the best means of obtaining the exact reproduction of indefinitely multiplied facsimiles of an original photograph, by which alone the publication of originals may be accomplished; and for which purpose the use of paper, or other similar materials, appears to be essentially requisite. In order to avoid circumlocution, the author employs the terms positive and negative to express, respectively, pictures in which the lights and shades are the same as in nature, or as in the original model, and in which they are the opposite; that is, light representing shade; and shade, light. The terms direct and reverse are also used to express pictures in which objects appear, as regards right and left, the same as in the original, and the contrary. In respect to photographic publication, the employment of a camera picture avoids the difficulty of a double transfer, which has been found to be a great obstacle to success in the photographic copying of engravings or drawings. The principal objects of inquiry to which the author has directed his attention in the present paper, are the following. First, the means of fixing photographs; the comparative merits of different chemical agents for effecting which, such as hyposulphite of soda, hydriodite of potash, ferrocyanate of potash, &c., he discusses at some length; and he notices some remarkable properties, in this respect, of a peculiar agent which he has discovered.


1. Lest the title of this communication should induce an expectation of its containing any regular and systematic series of researches developing definite laws, or pointing to any distinct theory of photographic action, it may be as well to commence it by stating its pretensions to be of a much lower kind, its object being simply to place on record a number of insulated facts and observations respecting the relations both of white light and of the differently refrangible rays to various chemical agents, which have offered themselves to my notice in the course of photographic experiments originating in the announcement of M. Daguerre’s discovery. The facts themselves, in the present state of our knowledge, will, I believe, be found by no means devoid of interest, and may lead, in the hands of others more favourably situated for such researches, and, I may add, in a better climate than ours, to inquiries of the utmost interest. 2. In a communication to this Society, which was read on the 14th of March, 1839, and of which an abstract will be found in the notices of its proceedings for that sitting, I have stated the circumstances which first directed my attention to this subject, and the progress I had then made, both in the scientific part of the inquiry and in its application to the photographic art. As that paper was (at my own request) withdrawn from the further immediate notice of the Society, and as the abstract alluded to may not fall into the hands of those who may read the present communication, a brief recapitulation of its contents will be necessary to preserve the connexion by which my inquiries have been linked together.


1998 ◽  
Vol 4 (S2) ◽  
pp. 216-217
Author(s):  
John T. Armstrong

Few quantitative analysis techniques attempt as large an extrapolation between the compositions of standards and samples than is attempted in electron microbeam x-ray emission analysis. In-situ x-ray microanalysis can be performed for essentially all elements in the periodic table in complex matricies that may contain, in extreme cases, thirty or more detectable elements. Analyses are attempted for the same elements, using the same standards, in various matrices whose average atomic numbers might range from 4 to 94. Unlike most analytical techniques, where suites of standards are synthesized having similar bulk compositions as the samples and bracketing the concentrations of the elements of interest, the standards employed in microbeam analysis are most commonly pure elements, simple oxides, or other binary element compounds. This is true even though matrix effects on electron retardation and scattering, x-ray absorption, and secondary x-ray fluorescence can cause major variations in the differences between relative intensity and relative concentration.


1888 ◽  
Vol 14 ◽  
pp. 125-129
Author(s):  
A. B. Griffiths ◽  
A. B. Griffiths

This paper details an investigation undertaken to see the influence of certain rays of white light on root-absorption and assimilation in the vegetable kingdom. One of us has been for some years investigating a problem as to the use of ferrous sulphate as a plant food (see Dr Griffiths' memoirs in Journal of Chemical Society [Trans.], 1883, 1884, 1885, 1886, 1887). In the experiments to be detailed here, we have used ferrous sulphate as an indicator of root-absorption.


Sign in / Sign up

Export Citation Format

Share Document