Access the full text.
Sign up today, get DeepDyve free for 14 days.
References for this paper are not available at this time. We will be adding them shortly, thank you for your patience.
LETTERS TO THE EDITOR Prompt publication of brief reports of important discoveries in physics may be secured by addressing them to this department. Closing dates for this depart- ment are, for the first issue of the month, the twenty-eighth of the preceding month; for the second issue, the thirteenth of the month. The Board of Editors does not hold itself responsible for the opinions expressed by the correspondents. The most stable configuiration, s2p4, of neutral oxygen gives rise to three terms, 3p, ID and 1S. McLennan' has shown that the green auroral line corresponds to the ID-IS transition. Recently Frerichs2 by a very exhaustive analysis of the oxygen spec- trum has been able to predict the positions of the 3P2-'D and 3P1-'D transitions at 6299 ±5A and 6363 ±5A respectively while a private communication to Dr. Frerichs from Professor Paschen states that he has found these lines in the laboratory at 6300.00A and 6363.86A. Wright's3 list of nebular lines shows weak unidentified lines at 6302A and 6364A. In agreement with the corresponding transitions in OiII the 3P2-1D line is two or three times as intense as the 3Pi-ID line. The general behavior of the lines in various nebulae
Physical Review – American Physical Society (APS)
Published: Aug 1, 1930
Read and print from thousands of top scholarly journals.
Already have an account? Log in
Bookmark this article. You can see your Bookmarks on your DeepDyve Library.
To save an article, log in first, or sign up for a DeepDyve account if you don’t already have one.
Copy and paste the desired citation format or use the link below to download a file formatted for EndNote
Access the full text.
Sign up today, get DeepDyve free for 14 days.
All DeepDyve websites use cookies to improve your online experience. They were placed on your computer when you launched this website. You can change your cookie settings through your browser.