4-8 July 2016
Kramer Law building
Africa/Johannesburg timezone
<a href="http://events.saip.org.za/internalPage.py?pageId=10&confId=86">The Proceedings of SAIP2016</a> published on 24 December 2017

Cosmic ray ground level enhancments: Power of pulse shape

6 Jul 2016, 14:00
20m
5B (Kramer Law building)

5B

Kramer Law building

UCT Middle Campus Cape Town
Oral Presentation Track D2 - Space Science Space Science

Speaker

Dr Olakunle Ogunjobi (Centre for Space Research, North-West University)

Apply to be<br> considered for a student <br> &nbsp; award (Yes / No)?

NO

Level for award<br>&nbsp;(Hons, MSc, <br> &nbsp; PhD, N/A)?

N/A

Abstract content <br> &nbsp; (Max 300 words)<br><a href="http://events.saip.org.za/getFile.py/access?resId=0&materialId=0&confId=34" target="_blank">Formatting &<br>Special chars</a>

Ground level enhancements (GLEs) of the cosmic-ray intensity have been observed 71 times since over seven decades. GLEs are due to sudden increases of solar energetic particles associated with large eruptive episodes. GLEs have been, controversially, divided into two distinct categories, gradual (classical) and impulsive events. Some recent findings argued that some GLEs are too impulsive to be accelerated in the eruptive episodes. Here we investigated this hypothesis by studying time profiles of ten GLEs, which were observed with excellent data coverage of associated solar eruptions. Preliminary results support that the shape of the profile is a
powerful indicator of propagation conditions between Sun and Earth. The average continuous range from gradual to impulsive will be presented

Please indicate whether<br>this abstract may be<br>published online<br>(Yes / No)

YES

Would you like to <br> submit a short paper <br> for the Conference <br> Proceedings (Yes / No)?

YES

Primary author

Dr Olakunle Ogunjobi (Centre for Space Research, North-West University)

Co-author

Dr Du Toit Strauss (Centre for Space Research, North-West University)

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