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
Related Articles
- EP ID EP395191
- DOI 10.9790/9622-0809051617.
- Views 131
- Downloads 0
Analysis of Packaging issues in current Electric vehicles.
The decade of 2020 is the decade for development of electric vehicle in automotive industries. The future of transportation is Electric vehicle as we are running out of Fossil fuels. The Global automotive industries are...
A Trident Extensible Multiprocessor Network
Recently the thrust for higher and higher computing power is increasing day by day, user don't miss an opportunity to use even there smaller and smaller laptop for this purpose to get their requirement full filled . As a...
Optimizing TCP Congestion Control techniques for modern Wireless Network
Transmission Control Protocol (TCP) intended to convey consistent and solid end-to-end information exchange crosswise over untrustworthy systems works perfectly well in wired condition. Indeed, TCP bears the 90% of Inter...
Convective Heat Transfer Model through Annular Finned Evaporator of a Cold Storage Using Taguchi Regression, S/N Ratio and ANOVA Analysis
To overcome the energy crisis and increase of cost of electrical energy to operate the cold storage various design of experiments are done to optimize different control factors of a cold storage evaporator space inside t...
Measuring of phase shift under polyharmonic signals condition
.