Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

  • Letter
  • Published:

Hydrogen in the Upper Atmosphere

Abstract

ONE of the most striking characteristics of both auroral and night-sky spectra is the absence of hydrogen lines. So far as I am aware, not even a trace of the atomic or molecular spectra of hydrogen has ever been observed in either of the above spectra. The question is immediately raised, does this absence prove that there is no hydrogen in the upper atmosphere at the heights at which night-sky and auroral spectra have been photographed? It is the purpose of this note to discuss briefly the answer to this question.

This is a preview of subscription content, access via your institution

Access options

Buy this article

Prices may be subject to local taxes which are calculated during checkout

Similar content being viewed by others

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

KAPLAN, J. Hydrogen in the Upper Atmosphere. Nature 136, 549–550 (1935). https://doi.org/10.1038/136549a0

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1038/136549a0

Comments

By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.

Search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing