Estimation of the solar proton spectrum in the GLE70 event

The GLE event on December 13, 2006 as observed by network station neutron monitor data is investigated (is considered). The GLE energetic spectrum suggested for this event is estimated taking into account the primary differential spectrum of galactic cosmic rays, coupling coefficients and integral m...

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Bibliographic Details
Published inAdvances in space research Vol. 43; no. 4; pp. 515 - 517
Main Authors Grigoryev, V.G., Starodubtsev, S.A., Dvornikov, V.M., Sdobnov, V.E.
Format Journal Article
LanguageEnglish
Published Elsevier Ltd 16.02.2009
Subjects
Coupling coefficients
Energy spectrum
Ground level enhancement
Integral multiplicities
Neutron monitor
Solar particle
Energy spectrum
Integral multiplicities
Neutron monitor
Solar particle
Ground level enhancement
Coupling coefficients
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Summary:The GLE event on December 13, 2006 as observed by network station neutron monitor data is investigated (is considered). The GLE energetic spectrum suggested for this event is estimated taking into account the primary differential spectrum of galactic cosmic rays, coupling coefficients and integral multiplicities of concrete detectors at different latitudes and levels of observation. It is noted that the additional increase of solar protons is also manifested in the ionization chamber ASK-1 data at the Yakutsk station.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0273-1177
1879-1948
DOI:10.1016/j.asr.2008.08.010