Authors: Z.S. Hamidi, Ungku Ferwani Salwa Ungku Ibrahim, Abidin, Z.Z, Ibrahim, Z.A., 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, Physics Division, Centre for Foundation Studies in Science, University of Malaya, 50603 Kuala Lumpur, Malaysia
Emails: [email protected]
Journal: International Journal of Fundamental Physical Sciences (IJFPS)
Volume: 3, Issue: 2, Pages: 20-23, Date: June, 2013
ISSN: 2231-8186
DOI: https://doi.org/10.14331/ijfps.2013.330048
This article broadly reviews our knowledge of theoretical solar radio burst type III (SRBT III) in the low frequency region. The eruption mechanism of solar flares and type III are currently an extremely active area of research. There is a focus on physical properties, models, and significant parameters relating to the behavior of bursts in low frequency. This review summarizes existing theories and aims to provide an understanding of SRBT III formation and behavior.
Solar radio burst type III (SRBT III), solar flare, Langmuir waves, Stochastic Growth theory