Atomic Emission Spectra of Neutral Noble Gases in the Infrared Spectral Range PDF Download
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Author: Svatopluk Civiš Publisher: Springer Nature ISBN: 303047352X Category : Science Languages : en Pages : 158
Book Description
This book is an invaluable guide to calibrating any infrared spectrum using noble gases as a reference. Featuring a detailed graphical and tabular overview of highly excited (Rydberg) states of neutral noble gases in the infrared range of 700–7000 cm-1, it helps researchers by providing high-precision experimental data that can be used in almost every infrared spectroscopic laboratory.
Author: Svatopluk Civiš Publisher: Springer Nature ISBN: 303047352X Category : Science Languages : en Pages : 158
Book Description
This book is an invaluable guide to calibrating any infrared spectrum using noble gases as a reference. Featuring a detailed graphical and tabular overview of highly excited (Rydberg) states of neutral noble gases in the infrared range of 700–7000 cm-1, it helps researchers by providing high-precision experimental data that can be used in almost every infrared spectroscopic laboratory.
Author: Ekaterina Zanozina Publisher: ISBN: 9783030473532 Category : Astronomy Languages : en Pages : 0
Book Description
This book is an invaluable guide to calibrating any infrared spectrum using noble gases as a reference. Featuring a detailed graphical and tabular overview of highly excited (Rydberg) states of neutral noble gases in the infrared range of 700-7000 cm-1, it helps researchers by providing high-precision experimental data that can be used in almost every infrared spectroscopic laboratory.
Author: William F. Meggers Publisher: Forgotten Books ISBN: 9780365164326 Category : Science Languages : en Pages : 28
Book Description
Excerpt from Infra-Red Spectra of Neon Argon and Krypton Neutral atoms of the noble gases are characterized by spectra of exceptional utility and rare beauty. Geissler tubes containing these gases at low pressure when excited by moderate electrical discharges, emit spectral lines of high homogeneity which have been demonstrated to be reproducible within 1 part in These lines are favor ably regarded as standards of wavelength, and are extensively used in spectroscopy and metrology. It is not unlikely that one of these lines may ultimately be chosen as the most practical and permanent primary standard of length, especially if an even-numbered isotope can be segregated so that the strongest lines will be free from hyperfine structure. From a theoretical viewpoint the first. Spectra of the noble gases are of special interest because they arise in each case from a; closed shell configuration of electrons, and unlike other complex spectra they are found to consist of extended series of relatively simple types terms) and low multiplicities (singlets and triplets). Evi dence of a gradual transition from sl to jj electron coupling as the atomic complexity increases adds interest to a comparison of the spectral structures of all the noble gases. 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.
Author: A. R. Striganov Publisher: Springer ISBN: Category : Science Languages : en Pages : 928
Book Description
Tables of Spectral Lines of Neutral and Ionized Atoms was first published in Moscow in 1966. All misprints and errors that have come to our attention have been corrected, and additions based on journal articles have been made for the Plenum Press edition. In particular, additions have been made in the tables for Li (4], C I [1], N I (1], N IV [12], and N V [14]. Such highly important spectra as those of N IV, NV, 0 IV, 0 V, and 0 VI in the visible and partially in the ultraviolet regions have, until recently, reƯ ceived almost no attention in the laboratory. The tables of these spectra inƯ clude astrophysical data from B. Edlen (Z. Astrophys., 7:378, 1933) and C.E. Moore (A Multiplet Table of Astrophysical Interest, Part I, N.B.S., 1945) with rather rough estimates of the wavelengths of the spectral lines. But as the spectra of highly ionized atoms have been studied in the laboratory, these values have been determined more precisely, and we have striven to incorporate them in the American edition of the book. For the spectra of N IV and NV, we have employed the recent, comprehensive papers of R. Hallin (Arkiv for Fysik, 32:201, 1966; 31:511, 1966), in which the system of energy levels was refined and expanded, and many classified lines in the visible, ordinary ultraƯ violet, and vacuum ultraviolet regions are cited.
Author: Svatopluk Civiš
Author: Svatopluk Civiš
Author: Ekaterina Zanozina
Author: William F. Meggers
Author: A. R. Striganov
Author: 
Author: David R. Lide
Author: 
Author: Richard Edward Stanley
Author: National Institute of Standards and Technology (U.S.)
Author: Rebecca J. Pardee