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The Astrophysical Journal
Article . 1979 . Peer-reviewed
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https://dx.doi.org/10.1086/182...
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On the solar coronal lines 1175-1965 A

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1979 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 227, page L107 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: G. D. Sandlin; R. Tousey;

doi: 10.1086/182878

On the solar coronal lines 1175-1965 A

Abstract

Sixteen new coronal lines are observed in ATM UV spectra. Identifications, wavelengths, and intensities are presented. Two additional lines observed previously are proposed as transitions within the 3p(3)3d configuration of Fe XI.

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    		 42
    popularity
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    		 Top 10%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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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).
BIP!Citations provided by BIP!
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.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
42
Top 10%
Top 10%
Top 10%
gold