Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Infrared Multiplets and the Solar Spectrum

Not Accessible

Your library or personal account may give you access

Abstract

The identification of solar lines in the photographic infrared region is discussed. Sample multiplets of C i, N i, O i, Na i, Al i, Si i, Ti i, and Fe i are listed to illustrate the consistency of term intervals within multiplets, when solar wave numbers are substituted for laboratory values. These data furnish an excellent criterion of both the precision of the solar data and the correctness of the assigned identifications. Solar lines produced by more than one contributor, i.e., blends, can be detected by irregularities in the solar term intervals within multiplets.

© 1953 Optical Society of America

Full Article  |  PDF Article
More Like This
Extension of the Second Spectrum of Zirconium into the Infrared

C. C. Kiess
J. Opt. Soc. Am. 43(11) 1024-1026 (1953)

The Magnesium Arc Spectrum in the Near Infrared*

Russell A. Fisher and Frances E. Eshbach
J. Opt. Soc. Am. 43(11) 1030-1032 (1953)

The Infrared Spectrum of Brucite [Mg(OH)2]*

R. T. Mara and G. B. B. M. Sutherland
J. Opt. Soc. Am. 43(11) 1100-1102 (1953)

Cited By

You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Tables (8)

You do not have subscription access to this journal. Article tables are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access Optica Member Subscription

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All Rights Reserved