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

Improved Determination of Source Temperature from Relative Spectrum Line Intensities

Not Accessible

Your library or personal account may give you access

Abstract

No abstract available.

Full Article  |  PDF Article
More Like This
Spectral-Line Intensities from Argon and Nitrogen Plasmas

L. E. Brewer, W. K. McGregor, and M. T. Dooley
J. Opt. Soc. Am. 52(7) 829_1-830 (1962)

Predicting the Distribution of Infrared Radiation from the Clear Sky

H. E. Bennett and Jean M. Bennett
J. Opt. Soc. Am. 52(11) 1305_1-1306 (1962)

Extreme Ultraviolet Reflection Spectrum of LiF†

W. C. Walker
J. Opt. Soc. Am. 52(2) 223-223 (1962)

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

Figures (1)

You do not have subscription access to this journal. Figure files 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

Equations (2)

You do not have subscription access to this journal. Equations 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