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

Infrared Spectroscopy of Planets and Stars

Not Accessible

Your library or personal account may give you access

Abstract

Infrared spectroscopy of the brighter planets and stars has been performed, and sample spectra of some objects are presented; the sensitivity limit for this purpose of scanning spectrometers is discussed. The spectrometer which has been used for three years is described. Advantages of a two-beam interferometer and its sensitivity increase are also presented.

© 1962 Optical Society of America

Full Article  |  PDF Article
More Like This
High Resolution Spectroscopy of Rotating Planets

T. J. Deeming and L. M. Trafton
Appl. Opt. 10(2) 382-385 (1971)

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 (6)

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

Tables (1)

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