Assessment of Seasonal Distribution and Characterisation of Geomagnetic Storm Occurrence during Solar Cycles 21–24

Authors

  • Moses Audu Department of Physics, Joseph Sarwuan Tarka University, P.M.B. 2373, Nigeria
  • Francisca Okeke Department of Physics and Astronomy, University of Nigeria, P.M.B. 410001, Nsukka, Enugu State, Nigeria
  • Tikyaa Emmanuel Department of Physics, Joseph Sarwuan Tarka University, P.M.B. 2373, Makurdi, Benue State, Nigeria
  • Jam Terkaa Department of Physics, Joseph Sarwuan Tarka University, P.M.B. 2373, Nigeria
  • Peter Onoja Department of Physics, Joseph Sarwuan Tarka University, P.M.B. 2373, Makurdi, Benue State, Nigeria
  • Inyope Thankgod Department of Physics, Joseph Sarwuan Tarka University, P.M.B. 2373, Makurdi, Benue State, Nigeria

DOI:

https://doi.org/10.52562/injoes.2024.1035

Keywords:

Geomagnetic storm, Dst index, seasonal distribution, space weather, solar cycle

Abstract

Geomagnetic storms (GMSs) are an important space weather phenomenon that poses serious threats to the advancement of space technology, power transmission lines, oil pipelines, and other infrastructure. This study investigates seasonal patterns of GMSs due to recent reports on the prominence of large storms (Dst ? -50 nT) during equinox conditions. Hourly Dst index data provided by the World Data Center, Kyoto, Japan, for solar cycles 21–24 (1976–2019) were employed. Storm occurrences in each solar cycle considered were identified using the minimum Dst value. The identified storms were categorized and analyzed statistically. Results revealed that storm occurrence varied from month to month, season to season, and solar cycle to solar cycle based on storm categories. Furthermore, the observed seasonal distribution of GMS occurrence decreases in the following order: autumn, spring, winter, and summer. This indicates that equinox conditions are more likely to have GMSs, consistent with the Russell-McPherron effect, compared to solstice conditions. The findings suggest that the distribution and characterization of storm occurrence vary seasonally due to solar activity. The insights on storm occurrence, distribution, and characterization may serve as a guide to space scientists to avert the impacts of GMSs while exploring space.

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References

Borovsky, J. E., & Denton, M. H. (2006). Differences between CME-driven storms and CIR-driven storms. Journal of Geophysical Research, 111(A7). https://doi.org/10.1029/2005JA011447

Chapman, S. C., Horne, R. B., & Watkins, N. W. (2020). Using the index over the last 14 Solar cycles to characterize extreme geomagnetic activity. Geophysical Research Letters, 47(3), e2019GL086524. https://doi.org/10.1029/2019GL086524

Christian, O. C. (2018). A statistical analysis of sunspot and CME parameters for the solar cycle 23. Physics and Astronomy International Journal, 2(4), 300?308. https://doi.org/10.15406/paij.2018.02.00103

Daglis, T., Konstantakis, K. N., & Michaelides, P. G. (2019). Solar events and economic activity: evidence from the US telecommunications industry (1996–2014). Physica A: Statistical Mechanics and its Applications, 534, 120805. https://doi.org/10.1016/j.physa.2019.04.041

Doha, A., & Wathiq, A. (2019). Large geomagnetic storms drive by solar wind in solar cycle 24, Journal of Physics: Conference Series, 1234, 012004. https://doi.org/10.1088/1742-6596/1234/1/012004

Gonzalez, W. D., Joselyn, J. A., Kamide, Y., Kroehl, H. W., Rostoker, G., Tsurutani, B. T. and Vasyliunas, V. M. (1994). What is a geomagnetic storm? Journal of Geophysical Research, 99, 5771. https://doi.org/10.1029/93JA02867

Gustavo, A. M. (2014). Solar cycle and seasonal distribution of geomagnetic storms with sudden commencement. Earth Science Research, 3(1), 50–55. https://doi.org/10.5539/esr.v3n1p50

Joshua, B. W., Oladipo, O. M., Adamu, J. L., Adebiyi, S. J., & Ikubanni, S. O. (2018). Correlation between sunspot number and geomagnetic storm. Equity Journal of Science and Technology, 5(1), 157-161.

Kane, R. P. (2014). Evolution of solar indices during the maximum of solar cycle 24. Indian Journal of Radio and Space Physics, 43, 151–155.

Kevser, K. (2021). Mathematical analysis of 08 May 2014 weak storm. Mathematics problems Engineer, 2021(1), 9948745. https://doi.org/10.1155/2021/9948745

Le, G.-M., Cai, Z.-Y., Wang, H.-N., Yin, Z.-Q., & Li, P. (2013). Solar cycle distribution of major geomagnetic storms. Research in Astronomy and Astrophysics, 13, 739–748. https://doi.org/10.1088/1674-4527/13/6/013

Love, J. J., Rigler, E. J., Pulkkinen, A., & Riley, P. (2015). On the lognormality of historical magnetic storm intensity statistics: Implications for extreme-event probabilities. Geophysical Research Letters, 42(16), 6544–6553. https://doi.org/10.1002/2015GL064842

Mandea, M., & Chambodut, A. (2020). Geomagnetic Field Processes and Their Implications for Space Weather. Survey Geophysics, 41, 1611–1627. https://doi.org/10.1007/s10712-020-09598-1

Mishra, P., Singh, U., Pandey, C. M., Mishra, P., & Pandey, G. (2019). Application of student's t-test, analysis of variance, and covariance. Annals of Cardiac Anaesthetia, 22(4), 407-411. https://doi.org/10.4103/aca.ACA_94_19

Parashar, K. K., Rathore, B. S., Kaushik, S. C., Kapil, P., & Gupta, D. C. (2011). Classification and study of geomagnetic storms during Year 1996-2010. International Journal of Pure and Applied Physics, 7(3), 199-202.

Ptitsyna, N. G., & Tyasto, M. I. (2017). Long-term trends and seasonal variations in geomagnetic storms from data of St. Petersburg Observatories (1878–1954). Geomagnetism and Aeronomy, 57, 1056–1062. https://doi.org/10.1134/S0016793217080205

Rashmi, P., Singh, S.B., & Kalyan, B. (2013). A study of seasonal variation of geomagnetic activity. Research Journal of Physical and Applied Sciences, 2(1), 1–011.

Rathore, B. S., Gupta, D. C., & Parashar, K. K. (2014). Relation between solar wind parameter and geomagnetic storm condition during cycle-23. International Journal of Geoscience, 5(13), 1602-1608. http://dx.doi.org/10.4236/ijg.2014.513131

Rathore, B.S., Kaushik, S. C., Bhadoria, R. S., Parashar, K. K., & Gupta, D. C. (2012). Sunspots and geomagnetic storms during solar cycle-23, Indian Journal of Physics, https://doi.org/10.1007/s12648-012-0106-2

Reyes, P. I., Pinto, V. A., & Moya, P. S. (2021). Geomagnetic Storm Occurrence and Their Relation with Solar Cycle Phases. Space Weather, 19(9), e2021SW002766. https://doi.org/10.1029/2021SW002766

Reyes, P., Pinto, V. A., & Moya, P. S. (2019). Statistical analysis of geomagnetic storms and their relation with the solar cycle. Proceedings of the International Astronomical Union, 15(S354), 224–227. https://doi.org/10.1017/S1743921320000903

Sawadogo, Y., Koala, S., & Zerbo, J. L. (2022). Factors of geomagnetic storms during the solar cycles 23 and 24: A comparative statistical study. Scientific Research and Essays, 17(3), 46-56. https://doi.org/10.5897/SRE2022.6751

Shadrina, L. P. (2017). Two types of geomagnetic storms and relationship between Dst and AE indexes. Solar-Terrestrial Relations and Physics of Earthquake Precursors. In E3S Web of Conferences (Vol. 20, p. 01010). EDP Sciences. https://doi.org/10.1051/e3sconf/20172001010

Svalgaard, L., Cliver, E. W., & Ling, A. G. (2002). The semiannual variation of great geomagnetic storms. Geophysical Research Letters, 29(16), 12-1-12-4. https://doi.org/10.1029/2001GL014145

Watari, S. (2017). Geomagnetic storms of cycle 24 and their solar sources. Earth, Planets and Space, 67, 70. https://doi.org/10.1186/s40623-017-0653-z

World Data Center for Geomagnetism, Kyoto. Nose, M., Iyemori, T., Sugiura, M., & Kamei, T. (2015). Geomagnetic Dst index. https://doi.org/10.17593/14515-74000

Wu, C., Liou, K., Lepping, R.P., Hutting, L., Plunkett, S., Howard, R. A., & Socker, D. (2016). The first super geomagnetic storm of solar cycle 24: “The St. Patrick’s day event (17 March 2015)”. Earth, Planets and Space, 68, 151. https://doi.org/10.1186/s40623-016-0525-y

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Published

2024-06-18

How to Cite

Audu, M., Okeke, F., Emmanuel, T., Terkaa, J., Onoja, P., & Thankgod, I. (2024). Assessment of Seasonal Distribution and Characterisation of Geomagnetic Storm Occurrence during Solar Cycles 21–24. Indonesian Journal of Earth Sciences, 4(1), A1035. https://doi.org/10.52562/injoes.2024.1035