Type III Radio Burst Emission and Sunspot Cycles
Journal Title: International Journal of engineering Research and Applications - Year 2018, Vol 8, Issue 9
Abstract
The paper considers the formation of type III solar radio bursts caused by plasma excitation and to examine the sunspot cycle length with an emphasis on the intervals between consecutive maxima and minima. From an elaborate analysis it appears that the most common cycle length is around 10.5 years, with few cycles in the range 11.5 to 12.5 years.
Authors and Affiliations
Debojyoti Halder, Bipasa Raha
Keywords
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- EP ID EP395191
- DOI 10.9790/9622-0809051617.
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