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Pergamos
Article . 2005
Data sources: Pergamos
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28 October 2003 flare: High-energy gamma emission, type II radio emission and solar particle observations

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2005 Greece Greek, Modern (1453-)
Authors: Kuznetsov, SN; Kurt, VG; Yushkov, BY; Myagkova, IN; Kudela; K; Belov, AV; +5 Authors

28 October 2003 flare: High-energy gamma emission, type II radio emission and solar particle observations

Abstract

The 28 October 2003 flare gave us the unique opportunity to compare the acceleration time of high-energy protons with the escaping time of those particles which have been measured onboard spacecraft and by neutron monitors network as GLE event. High-energy emission time scale and shock wave height and velocity time dependencies were also studied.

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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!
0
Average
Average
Average
Green
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