Variation of Solar Activity Parameters with Cosmic Ray intensity and Comparison of Solar Cycle 23-24

Authors

  • Shabir Ahmad  Department of Physics, A. P. S.University Rewa Madhya Pradesh, India
  • P. R. Singh  Department of Physics, A. P. S.University Rewa Madhya Pradesh, India
  • A. K. Saxena  Department of Physics, A. P. S.University Rewa Madhya Pradesh, India
  • C. M. Tiwari  Department of Physics, A. P. S.University Rewa Madhya Pradesh, India

Keywords:

cosmic rays, sunspot number, total solar irradiance, interplanetary magnetic field

Abstract

In this paper we have studied a significant relation between Cosmic Ray Intensity (CRI) and Solar activity parameter. The study is extended to solar cycle 23-24. In the present work, yearly average of Sunspot number (SSN), Total solar irradiance (TSI) and magnetic field (B) have been used to correlate with yearly average cosmic ray intensity. Comparison has been drawn between the successive solar cycles and it has been noticed that for two solar cycles the cosmic ray intensity is anti correlated with sunspot number, Total solar irradiance and magnetic field. We find the correlation coefficient of cosmic ray intensity with sunspot number as well as Total solar irradiance which are relatively large and anti correlated during solar cycle 23-24. However the magnetic field shows a positive correlation with Total solar irradiance and sunspot number and correlation coefficient for sunspot number and Total solar irradiance is R= 0.80 for solar cycle 23-24. While as interplanetary magnetic field is significantly correlated with sunspot number and value of correlation coefficient is 0.61.

References

  1. Haigh, J.: 2007, The Sun and the Earth’s Climate, Living Rev. Solar Phys. 4, 2. doi: 10.12942/lrsp- 2007-2.
  2. Eddy, J.: 1976, The Maunder Minimum, Science 192, 4245.
  3. Ermolli, I., Matthes, K., Dudok de Wit, T., Krivova, N.A., Tourpali, K., Weber, M., et al.: 2013, Recent variability of the solar spectral irradiance and its impact on climate modelling, Atmos. Chem. Phys.,13, 394. doi:10.5194/acp-13-3945-2013.
  4. Solanki, S.K., Krivova, N.A., Haigh, J.D.: 2013, Solar Irradiance Variability and Climate, Annu. Rev. Astron. Astrophys. 51, 1056-8700/97/0610-00.
  5. Axford, W. I. (1965). Anisotropic diffusion of solar cosmic rays. Planet. Space Sci.,13, pp. 1301–+.
  6. A. J. Hundhausen. Coronal Expansion and Solar Wind. 1972.
  7. M. G. Kivelson and C. T. Russell. Introduction to Space Physics. April 1995.
  8. E. N. Parker. Dynamics of the Interplanetary Gas and Magnetic Fields. ApJ ,
  9. E. N. Parker. Dynamical Theory of the Solar Wind. Space Sci : Rev: , 4:666-708, September 1965.
  10. T. I. Gombosi, editor. Physics of the space environment, 1998.
  11. L. Biermann, B. Brosowski, and H. U. Schmidt. The interactions of the solar wind with a comet. Sol:P hys: , 1:254{284, March 1967.
  12. Hickey, J. R., B. M. Alton, F. J. Griffin, H. Jacobowitz, P.Pellegrino, E. A. Smith, T. H. Vonder Haar, and R. H. Maschhoff, 1981

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Published

2017-12-31

Issue

Section

Research Articles

How to Cite

[1]
Shabir Ahmad, P. R. Singh, A. K. Saxena, C. M. Tiwari, " Variation of Solar Activity Parameters with Cosmic Ray intensity and Comparison of Solar Cycle 23-24, International Journal of Scientific Research in Science, Engineering and Technology(IJSRSET), Print ISSN : 2395-1990, Online ISSN : 2394-4099, Volume 3, Issue 8, pp.324-327, November-December-2017.