Excerpt from Interference Measurements of Wave Lengths in the Iron Spectrum, 3233a-6750a
Seed 27 plates were used throughout, but to photograph the region 4900a to 67 50a the plates were'bathed in pinaverdol and dicyanin with ammonia. In the region 32'o0a to 4200a there were measured: Four exposures of 1; five of 6; one each of 15, 20, and 30; and two of 60' minutes' duration. In the region 3 500a to 4500a the exposures were: Five of 2; five of 5 two of 20; and three of 25 minutes. The region 4100a to 5100a was covered by exposures as follows: Three of 3; two of 5; one of 10; four of 15; one of 25; and four of 50 minutes. Finally, in the region 4900a to 6800a, the following exposures were measured: One of 1; two of 3; three of 5; three of 9; two of 15; three of 20; two of 90; and one each of 65, 80, and 100 minutes' duration. The first three regions were photographed in the second order; 4900a to 6800a was taken in the first order. In almost every case two or more exposures were measured on the same plate.
These exposures were made without disturbing the interferome ter. In 3 cases out of 24 there Was a change in the thickness of about one part in a million, and in a few other cases there was a barely perceptible change. These changes'were probably due to a variation in the temperature, although the thermometer beside the interferometer registered no appreciable change. By allow ing the light to fall upon the interferometer for half an hour before taking the plate this trouble could be avoided. A short exposure was always made first, and another short exposure usually followed the long one. In any case, each exposure was worked out by itself and this expansion of the interferometer caused no difficulty. In a few cases the long exposure on a plate was too dense to permit of accurate measurement of a sufficient number of standards. In such cases the long and short exposures were tied together-by lines of intermediate intensity. It will be seen at once that this method would lead to' erroneous results in case there were an intensity equation. The question will be discussed later in connection with the grating observations.
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Excerpt from Interference Measurements of Wave Lengths in the Iron Spectrum, 3233a-6750a
Seed 27 plates were used throughout, but to photograph the region 4900a to 67 50a the plates were'bathed in pinaverdol and dicyanin with ammonia. In the region 32'o0a to 4200a there were measured: Four exposures of 1; five of 6; one each of 15, 20, and 30; and two of 60' minutes' duration. In the region 3 500a to 4500a the exposures were: Five of 2; five of 5 two of 20; and three of 25 minutes. The region 4100a to 5100a was covered by exposures as follows: Three of 3; two of 5; one of 10; four of 15; one of 25; and four of 50 minutes. Finally, in the region 4900a to 6800a, the following exposures were measured: One of 1; two of 3; three of 5; three of 9; two of 15; three of 20; two of 90; and one each of 65, 80, and 100 minutes' duration. The first three regions were photographed in the second order; 4900a to 6800a was taken in the first order. In almost every case two or more exposures were measured on the same plate.
These exposures were made without disturbing the interferome ter. In 3 cases out of 24 there Was a change in the thickness of about one part in a million, and in a few other cases there was a barely perceptible change. These changes'were probably due to a variation in the temperature, although the thermometer beside the interferometer registered no appreciable change. By allow ing the light to fall upon the interferometer for half an hour before taking the plate this trouble could be avoided. A short exposure was always made first, and another short exposure usually followed the long one. In any case, each exposure was worked out by itself and this expansion of the interferometer caused no difficulty. In a few cases the long exposure on a plate was too dense to permit of accurate measurement of a sufficient number of standards. In such cases the long and short exposures were tied together-by lines of intermediate intensity. It will be seen at once that this method would lead to' erroneous results in case there were an intensity equation. The question will be discussed later in connection with the grating observations.
About the Publisher
Forgotten Books publishes hundreds of thousands of rare and classic books. Find more at www.forgottenbooks.com
This book is a reproduction of an important historical work. Forgotten Books uses state-of-the-art technology to digitally reconstruct the work, preserving the original format whilst repairing imperfections present in the aged copy. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in our edition. We do, however, repair the vast majority of imperfections successfully; any imperfections that remain are intentionally left to preserve the state of such historical works.
Excerpt from Interference Measurements of Wave Lengths in the Iron Spectrum, 3233a-6750a
The differences, Grating minus B. S., were taken for each series and these data were collected for each 200a. In 5 out of these 13 regions the algebraic means for the best grating measure ments agreed in showing a difference between the B. S. And the grating scale. This is no doubt due in part to an accumulation of errors of like sign in the B. S. Table, and in part to the fact that the grating follows the local standards much more closely than does the interferometer. Further, the grating observers used some manganese standards and some iron standards which were too poor to be observed on our plates. The greatest difference is 0.0019a in the region 6200a to 6400a.
About the Publisher
Forgotten Books publishes hundreds of thousands of rare and classic books. Find more at www.forgottenbooks.com
This book is a reproduction of an important historical work. Forgotten Books uses state-of-the-art technology to digitally reconstruct the work, preserving the original format whilst repairing imperfections present in the aged copy. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in our edition. We do, however, repair the vast majority of imperfections successfully; any imperfections that remain are intentionally left to preserve the state of such historical works.
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Paperback. Condición: New. Print on Demand. This book details the author's quest to meticulously measure and record the wavelengths of iron spectrum lines to create a definitive standard. The author's work builds upon the work of previous scientists, and contributes to the overall effort to create a comprehensive and accurate map of the iron spectrum. The insights gained from this book have been indispensable in advancing our understanding of the behavior of iron under different conditions, and have applications in astrophysics and other fields. This book is a reproduction of an important historical work, digitally reconstructed using state-of-the-art technology to preserve the original format. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in the book. print-on-demand item. Nº de ref. del artículo: 9781334262449_0
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PAP. Condición: New. New Book. Shipped from UK. Established seller since 2000. Nº de ref. del artículo: LW-9781334262449
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PAP. Condición: New. New Book. Shipped from UK. Established seller since 2000. Nº de ref. del artículo: LW-9781334262449
Cantidad disponible: 15 disponibles