Abstract
THE Lyman lines of hydrogen, as well as the corresponding lines of He I and He II, are of interest both as tools for analysing the solar atmosphere and as energy sources for the terrestrial ionosphere. So far, interest in these lines has centred mainly around the Lyman-α lines because of their greater strength.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
