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Solar Activity Changes During Prolonged Sunspot Minima as Inferred from Indian Monsoon Rainfall Variations

Published online by Cambridge University Press:  27 November 2018

S. Ambily ,
V. G. Haritha ,
C. Sunil Kumar Morais  and
T. E. Girish
S. Ambily
Affiliation:
Department of Physics, University College, Trivandrum 695034, India emails: ambilysuresh03@gmail.com, vgharithamanoj@gmail.com, tegirish5@yahoo.co.in
V. G. Haritha
Affiliation:
Department of Physics, University College, Trivandrum 695034, India emails: ambilysuresh03@gmail.com, vgharithamanoj@gmail.com, tegirish5@yahoo.co.in
C. Sunil Kumar Morais
Affiliation:
PhD Research scholar in Physics, M.S. University, Tirunelveli, India email: sunilkumarmoraisc@yahoo.co.in
T. E. Girish
Affiliation:
Department of Physics, University College, Trivandrum 695034, India emails: ambilysuresh03@gmail.com, vgharithamanoj@gmail.com, tegirish5@yahoo.co.in
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Abstract

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We could find a new 5 year periodicity in the occurrences of peaks in sunspot activity and inferred deviations of annual Indian monsoon rainfall variations from the normal during the Maunder minimum (MM) period. This result is explained in terms of solar dynamo functioning in a different mode from normal during the MM where quadrupole field (first harmonic, 5-5.5 years) dominate over dipole field (fundamental, 11 years) causing extreme north south asymmetry in sunspot activity.

Keywords

Maunder minimaIndian monsoon rainfall5.5 year periodicitysolar activitysolar dynamoquadrupole fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 209 - 210
Copyright
Copyright © International Astronomical Union 2018 

References

Eddy, J. A., 2012, Science, 192, 1189–1202Google Scholar
Hiremath, K. M., Manjunath, H., & Soon, W., 2015, NewAstron, 35, 8–19Google Scholar
Mertens, M. T. 2003, 17&18 century Dutch shipping records unveil ENSO signals in the Indian Ocean, MA Thesis, California State University, USA.Google Scholar
Uberoi, C., 2012, EOS, 93, 437–438Google Scholar
Vaquero, J. M., Kovaltsov, G. A., Usoskin, I. G., Carrasco, V. M. S., & Gallego, M. C., 2015a, A&A, 577, A71Google Scholar
Vaquero, J. M., Nogales, J. M., & Bajo, F. S. 2015b, arXiv:1501.05989 [astro-ph.SR]Google Scholar
Vazquez, M., Vaquero, J. M., Gallego, M. C., Cartes, T. R., & Palle, P. L., 2016, Sol. Phys., 291, 616–642Google Scholar