Proceedings Paper
Upgrading the database by Fourier transform spectrometry| Format | Member Price | Non-Member Price |
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Paper Abstract
Current work with the visible-UV FT spectrometer at Imperial College is directed at improving the data base for the astrophysically and analytically important transition elements, using complementary data from the IR obtained at the National Solar Observatory, starting with iron, chromium and cobalt. This paper highlights the gains and problems of FTS for this type of work.
Paper Details
Date Published: 1 March 1992
PDF: 2 pages
Proc. SPIE 1575, 8th Intl Conf on Fourier Transform Spectroscopy, (1 March 1992); doi: 10.1117/12.56453
Published in SPIE Proceedings Vol. 1575:
8th Intl Conf on Fourier Transform Spectroscopy
Herbert Michael Heise; Ernst Heiner Korte; Heinz W. Siesler, Editor(s)
PDF: 2 pages
Proc. SPIE 1575, 8th Intl Conf on Fourier Transform Spectroscopy, (1 March 1992); doi: 10.1117/12.56453
Show Author Affiliations
R. C. Learner, Imperial College of Science, Technology and Medicine (United Kingdom)
G. Nave, Imperial College of Science, Technology and Medicine (United Kingdom)
J. E. Murray, Imperial College of Science, Technology and Medicine (United Kingdom)
G. Nave, Imperial College of Science, Technology and Medicine (United Kingdom)
J. E. Murray, Imperial College of Science, Technology and Medicine (United Kingdom)
Juliet Pickering, Imperial College of Science, Technology and Medicine (United Kingdom)
Anne P. Thorne, Imperial College of Science, Technology and Medicine (United Kingdom)
James W. Brault, National Solar Observatory (United States)
Anne P. Thorne, Imperial College of Science, Technology and Medicine (United Kingdom)
James W. Brault, National Solar Observatory (United States)
Published in SPIE Proceedings Vol. 1575:
8th Intl Conf on Fourier Transform Spectroscopy
Herbert Michael Heise; Ernst Heiner Korte; Heinz W. Siesler, Editor(s)
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