Kα Satellite Lines

Clicks: 2
ID: 269883
1936
Free PDF
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This article has not been analysed, so there is no overall score — reader engagement is measured and shown alongside.
AI Quality Assessment
Not analyzed
Readership in this journal
Popular

Ranked #17 of 17 articles by views in physical review

Most read Least read

Bar heights use a square-root scale.

Mint this article as an NFT
Not yet minted

Create a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.

5 SUSD one-off · no wallet required
Sign in to mint
Abstract
With a two-crystal vacuum spectrometer, ionization curves of the $K{\ensuremath{\alpha}}_{3, 4}$ group of x-ray satellite lines have been recorded for elements S(16) to Ge(32). In the $K{\ensuremath{\alpha}}_{3, 4}$ satellite group are found five component lines for $16\ensuremath{\le}Z\ensuremath{\le}28$ and four components for $29\ensuremath{\le}Z\ensuremath{\le}32$. The wave-length position, relative intensity, and line width at half-maximum intensity of each satellite component has been measured. The widths and shapes of the $K{\ensuremath{\alpha}}_{1, 2}$ lines were determined and a brief discussion of these data is given.
Reference Key
parratt1936physicalkα Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Lyman G. Parratt;
Journal physical review
Year 1936
DOI
doi:10.1103/PhysRev.50.1
URL
https://doi.org/10.1103%2FPhysRev.50.1
Keywords

Citations

No citations found. To add a citation, contact the admin at info@scimatic.org

Comments

No comments yet. Be the first to comment on this article.