Solar abundance of praseodymium

descriptionPublicationkeyboard_double_arrow_right Article 01 Feb 1979 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 61, pages 17-22 (issn: 0038-0938, eissn: 1573-093X,

Copyright policy )

Authors: Emile Bi�mont; Nicolas Grevesse; �ivind Hauge;

doi: 10.1007/bf00155442

Solar abundance of praseodymium

- Summary
- Metrics

Abstract

16 lines of Pr ii possibly present in the solar photospheric spectrum have been studied. When including hyperfine structure in synthetic calculations, investigations of 9 lines result in an abundance APr = 0.71 ± 0.08 in the log AH = 12.00 scale.

Related Organizations

University of Oslo
Norway
University of Liège
Belgium

Impact byBIP!

	selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	7
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average