Iranian Journal of Geophysics

Iranian Journal of Geophysics

Analyzing the relationship between solar magnetic polarity, solar wind velocity, and vertical magnetic field (Bz)

Document Type : Research Article

Authors
1 Ph.D. Student, Research Scholar, Department of Physics, Women’s Christian College, Nagercoil, India
2 Associate Professor, Department of Physics and Research Centre, Women’s Christian College, Nagercoil, India
Abstract
This study examines the influence of solar magnetic polarity and solar wind velocity on the
Bz-component of the interplanetary magnetic field (IMF Bz) during the solar cycles 22, 23, 24, and 25, characterized by the minimum of solar activity. The analysis reveals a distinctive pattern in the behavior of the solar magnetic field. Specifically, during even solar cycles (22 and 24), the solar magnetic field exhibits an opposite polarity, while in odd solar cycles (23 and 25), it demonstrates a positive polarity. This finding supports the formulation of an odd-even hypothesis, which is further corroborated by the qualitative analysis of IMF Bz to other factors such as IMF Bx, solar wind velocity, and the polarity of the Sun's magnetic field. Our investigation reveals that IMF Bz is significantly influenced by the polarity of the Sun's magnetic field, solar wind velocity, and the magnitude of the IMF horizontal component (Bx). Moreover, we find a positive correlation between IMF Bz and both Bx and solar wind velocity, regardless of the magnetic field polarity being positive or negative. These findings contribute to our understanding of the interplay between solar magnetic activity, solar wind dynamics, and the behavior of the interplanetary magnetic field during periods of minimum solar activity. The dependencies observed in this study offer valuable insights into the complex nature of solar-terrestrial interactions. Furthermore, they hold implications for studying the effects of solar variability on Earth's magnetosphere. By comprehending the relationships between solar magnetic activity, solar wind properties, and the behavior of the interplanetary magnetic field, scientists can gain a deeper understanding of the dynamics involved in the interaction between the Sun and the Earth's magnetic field. This research sheds light on the factors influencing the IMF Bz and provides a foundation for further investigations in this field. With the continuously advancing knowledge in solar physics and space weather, these findings contribute to the broader scientific understanding of our solar system and its effects on our planet. Further studies building upon these insights may aid in predicting and mitigating the potential impacts of solar variability on various technological systems and the Earth's space environment. This study contributes to the scientific understanding of the influence of solar magnetic polarity and solar wind velocity on the interplanetary magnetic field. The observed patterns and correlations provide valuable insights into the dynamics of solar-terrestrial interactions, paving the way for further research in the field of space weather and its impacts on Earth.
Keywords

Subjects


Antonucci, E., Marocchi, D. “Heliographic-latitude dependence of the cosmic-ray intensity”, Geophys. Res. Lett. 1, 302, 1974.
Babcock, H. D., “The sun's polar magnetic fields”, Astrophys. J., 13, 364, 1959.
Barker, M.C., Hatton, G.J. “Evidence for a cosmic ray gradient perpendicular to the solar equatorial plane” Journal of  Planet Space Science Vol. 19, pp.549, 1971.
Balogh, A., Forsyth, R. J., Lucek, E. A., Horbury, T. S., and Smith, E. J. “ Heliospheric magnetic field polarity inversions at high heliographic latitudes”, Geophys. Res. Lett., 26, 631–634, 1999.
Berti, R., M. Laurenza, G. Moreno, and M. Storini, “Interplanetary magnetic field polarities derived from measurements of the northern and southern polar geomagnetic field”, J. Geophys. Res., 2006.
Crooker, N.U., Lazarus, A.J., Phillips, J.L., Steinberg, J.T., Szabo, A., Lepping, R.P., Smith, E.J. Coronal streamer belt asymmetries and seasonal solar wind variations deduced from Wind and Ulysses data. J. Geophys. Res. 102, 4673, 1997.
Dessler, A. J., “Solar wind and interplanetary magnetic field”, Rev. Geophys. Space Phys., 5, l, 1967.
Forsyth, F. J., Balogh, A., Horbury, T. S. and Smith, E. J. “The heliospheric magnetic field at solar minimum as observed by ULYSSES”, Adv. Space Res., 19, 839–842, 1997.
Forsyth, B. and Breen, A. “The 3D Sun and heliosphere at solar maximum”, meeting report, Astron. Geophys., 43(3), p. 3.32., doi:10.1046/j.1468-4004.2002.43332.x, 2002.
Fougere, P. E., “Dependence of inferred magnetic sector structure upon geomagnetic and solar activity”, Planet. Space Sci., 22, 1173–1184, 1974.
Gazis, P.R “The latitudinal structure of the solar wind in the solar equator near solar minimum: 1986 and predictions for 1997”. Journal of Geophysics, Vol 24, pp.627, 1997.
Gonzalez, W. D., and B. T. Tsurutani, “Criteria of interplanetary parameters causing intense magnetic storms (Dst < 100 nT)” Journal of Planet. Space Sci., Vol 35, pp.1101, 1987.
Gosling, J.T., Bame, S.J., McComas, D.J., Phillips, J.L., Pizzo, V.J., Goldstein, B.E., Neugebauer, M. Latitudinal variation of solar wind corotating stream interaction regions: Ulysses. Geophys. Res. Lett. 20 (24), 2789–2792, 1993.
Hirshberg, J., “The transport of flare plasma from the sun to the earth”, Planet. Space Sci., 16, 309, 1968.
Hirshberg, J., “Interplanetary magnetic field during the rising part of the solar cycle”, J. Geophys. Res., 74, 5814, 1969.
Howard, R., Polar magnetic fields of the sun: 1960-1971, Solar Phys., 25, 5, 1972.
Jokipii, J. R., “Propagation of cosmic rays in the solar wind”, Rev. Geophys. Space Phys., 9, 27, 1971.
Kamide, Y., et al., “Current understanding of geomagnetic storms: Storm substorm relationship”, Journal of Geophysical Research, Vol. 103, pp.705, 1998.
King, J. H., “A survey of long-term interplanetary magnetic field variations”, J. Geophys. Res., 81,653, 1976.
Kyung-Eun Choi and Dae-Young Lee, “Origin of Solar Rotational Periodicity and Harmonics Identified in the Interplanetary Magnetic Field Bz Component Near the Earth During Solar Cycles 23 and 24”, Journal of Solar Physics, Vol. 294:44, 2019.
Lyatsky, W., Tan, A., Lyatskaya, S. “Effect of Solar magnetic field polarity on interplanetary magnetic field Bz”. Geophys. Res. Lett. 30 (24), 2258, 2003.
Pizzo, V. J., “Global, quasi-steady dynamics of the distant solar wind, 2, Deformation of the heliospheric current sheet”, Journal of Geophys. Res., 99, 4185, 1994.
Ponyavin, D. I, “Retrieval of the polarity of the interplanetary magnetic field in the past”, Geomagn. Aeron., 31, 1094–1096, 1991.
Rosenberg, R.L., Coleman, P.J. “Heliographic latitude dependence of the dominant polarity of the interplanetary magnetic field” Journal of Geophysical Research, Vol.74, pp.5611, 1969.
Russell, C. T., On the heliographic latitude dependence of the interplanetary magnetic field as deduced from the 22-year cycle of geomagnetic activity, Geophys. Res. Lett., 1, 1 l, 1974.
Smith, E. J., “The Pioneer-Jupiter magnetic field investigation”, Tech. Rep. 616-48, Jet Propul. Lab., Pasadena, Calif., 1973.
Simon Wing and David G. Sibeck, “Effects of interplanetary magnetic field z component and the solar wind dynamic pressure on the geosynchronous magnetic field”, Journal of geophysical research, Vol. 102, pp.7207-7216, 1997.
Takao Aoki, “Influence of the interplanetary magnetic field on the ring current injection rate” Journal of Earth Planets Space, Vol.58, pp. 679–688, 2006.
Tritakis, Basil P. “A solar cycle variation of the interplanetary magnetic field configuration”. Solar Phys. 63, 207–215, 1979.
Velli M and  Pruneti F, “Alfven waves in the solar corona and solar wind”, Plasma Phys. Control. Fusion, 39, B-317, 1997.
Wilcox, J. M., and P. H. Scherrer, “Annual and solar magnetic cycle variations in the interplanetary magnetic field, 1926-1971”, J. Geophys. Res., 5385, 1972.