Authors: Z.S. Hamidi, Z.Z. Abidin, Z.A. Ibrahim, C. Monstein, N.N.M. Shariff
Affiliations: Department of Physics, Faculty of Science, University of Malaya, 50603 Kuala Lumpur, Malaysia, Faculty of Applied Sciences, MARA University of Technology, UiTM 40450 Shah Alam Selangor, Malaysia, Institute of Astronomy, ETH, Zurich, Switzerland
Emails: [email protected]
Journal: International Journal of Fundamental Physical Sciences (IJFPS)
Volume: 2, Issue: 3, Pages: 32-34, Date: September, 2012
ISSN: 2231-8186
DOI: https://doi.org/10.14331/ijfps.2012.330032
This review intended to update the results of combination two burst, type III and V in one solar flare event. Magnetic reconnection of both burst will be explained theoretically. Both bursts are found on 19th September 2011 associated with C-class flares on active region 1295. [...] Although the sources of both bursts are same, the direction and ejection explode differently. It is believed that the ejection of particles in type III burst is more compare type V. In summary, the behavior of type III should be critically understood in order to predict the formation of type V burst.
Solar radio burst, solar flare, type III, type V, CALLISTO