Type III Radio Burst Emission and Sunspot Cycles

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.
  • Views 138
  • Downloads 0

How To Cite

Debojyoti Halder, Bipasa Raha (2018). Type III Radio Burst Emission and Sunspot Cycles. International Journal of engineering Research and Applications, 8(9), 16-17. https://europub.co.uk/articles/-A-395191