On the relationship between ground level enhancement and solar flare

Details On the relationship between ground level enhancement and solar flare On the relationship between ground level enhancement and solar flare

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jgra..11604101f&link_type=abstract

Journal of Geophysical Research, Volume 116, Issue A4, CiteID A04101

Astronomy and Astrophysics

Astrophysics

2

Interplanetary Physics: Cosmic Rays, Interplanetary Physics: Energetic Particles (7514), Interplanetary Physics: Solar Cycle Variations (7536), Solar Physics, Astrophysics, And Astronomy: Flares, Solar Physics, Astrophysics, And Astronomy: Coronal Mass Ejections (2101)

Scientific paper

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, on average, the GLE event-associated solar flare (˜0.2 × 10-4 W/m2) is much stronger than the non-GLE-associated solar flare (˜0.3 × 10-5 W/m2). The findings have also been supported by the solar flare indices that, on average, the GLE event-associated solar flare index (˜35.01) is much higher than the non-GLE-associated solar flare index (˜4.88). However, this association does not seem to precisely imply that GLEs can occur because of a solar flare, so we examined cross correlations between GLE events and simultaneous solar flares. We found that most (˜78%) of the highest correlations (r > 0.8) took place during an X class flare. There is no clear indication that the more the time lag, the less or more is the correlation or vice versa. Overall, 50% of the high correlations took place at higher time lag (≥65 min), and ˜36% of the high correlations took place at lower time lag (≤40 min), while the rest (˜14%) of the correlations were abruptly high and low at medium time lag (>40 and <65 min). On the basis of the results of cross correlations, we suggest that the intensive portions of solar flares should be responsible for causing GLEs and that the direct proportionality of the time-integrated intensive portion of a flare with the impulsive phase of a GLE event seems to be the main property for comprehending the mechanism.

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