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Article . 1990
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Astrophysics and Space Science
Article . 1990 . Peer-reviewed
License: Springer TDM
Data sources: Crossref
https://dx.doi.org/10.1007/bf0...
Article
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Coronal line intensity as an integrated index of solar activity

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1990 Greece English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 164, pages 117-130 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )
Authors: Xanthakis, J.; Petropoulos, B.; Mavromichalaki, H.;

doi: 10.1007/bf00653557

Coronal line intensity as an integrated index of solar activity

Abstract

The relation between coronal green line intensity and high-speed streams of solar wind emitted by coronal holes or by loop structures of the corona is studied. As well as these exclusive regions of coronal radiative emission, other factors of solar activity have been taken into account in this relation, such as proton events, sunspot number, faculae, and solar magnetic fields.

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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!
10
Average
Top 10%
Average
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