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Titel Relationship between GLE and Solar X-ray Flare
VerfasserIn Kazi Abul Firoz, Yong-Jae Moon, Kyung-Suk Cho, Jung-A Hwang, Yong-Deuk Park, Karel Kudela, Lev Dorman
Konferenz EGU General Assembly 2011
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 13 (2011)
Datensatznummer 250050115
 
Zusammenfassung
We made an effort to understand the associations and relationships between ground level enhancement (GLE) events and solar flares for the time period of 1986 – 2006. Our results show that, averagely, the GLE-event associated solar flare (~ 0.2 x 10-4 w/m2) is much stronger than non-GLE associated solar flare (~ 0.3 x 10-5 w/m2). The findings have also been supported by the solar flare indices that, averagely, the GLE-event associated solar flare index (~ 35.01) is much higher than the non-GLE associated solar flare index (~ 4.88). Yet, this association does not seem to precisely imply that GLE can be occurred by solar flare, so we examined cross-correlations between GLEs and simultaneous solar flares. We found that most (~78%) of the highest correlations (r>0.8) took place during X-class flare. There is no clear indication that the more the time-lag, the less or more is the correlation or vice-versa. On overall, 50% high correlations took place at higher time delay (-‰¥65 min) and ~36% high correlations took place at lower time-delay (-‰¤40 min) while the rest (~14%) of the correlations were abruptly high and low at medium time-delay (>40,