Abstract
This paper investigates the North–South (N–S) as well as East–West (E–W) distribution and asymmetry in Soft X-ray flares (SXR) activity during the period 1976–2019 which corresponds to solar cycles 21–24. Our results reveal that, cycles 21, 22 and 23 are dominated by southern hemisphere and the cycle 24 is also found to be southern hemisphere dominated using soft X-ray flares data. The cumulative plot indicates a slight excess of X-ray flare events in the southern hemisphere during solar cycles 21, 23 and 24. A significant excess of flare events in the southern hemisphere has been observed in the cumulative plot during cycle 22. The most prolific latitude band in the N–S distribution is the 10°–20° which produced maximum number of soft X-ray flares over solar cycles 21, 22, 23 and 24 whereas no such longitudinal band is observed in the E–W distribution. The time-latitude plot of SXR flares is also constructed to study the behaviour of N–S distribution. It is also revealed in current work that the occurrence (number) of M and X class flares is showing a declining trend since solar cycle 21 till solar cycle 24 thereby violating the Gnevyshev-Ohl (G-O) rule. A significant eastern dominance is being observed till solar cycle 23 but the predominance shifted to western hemisphere during cycle 24. Our analysis reveals that the North–South asymmetry is highly significant in comparison to East–West asymmetry.
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REFERENCES
Badalyan, O.G., Spatial distribution of the N–S asymmetry of solar activity and its time variations, Astron. Lett., 2012, vol. 38, pp. 51–61. https://doi.org/10.1134/S1063773711120024
Badalyan, O.G. and Obridko, V.N., North–south asymmetry of solar activity as a superposition of two realizations: The sign and absolute value, Astron. Astrophys., 2017, vol.603, pp. A109–A119.https://doi.org/10.1051/00046361/201527790
Bai, T., Distribution of flares on the sun during 1955–1985, Astrophys. J., 1987, vol. 314, pp. 795–807. https://doi.org/10.1086/165105
Bai, T., Distribution of flares on the Sun: Superactive regions and active zones of 1980–1985, Astrophys. J., 1988, vol. 328, pp. 860–874. https://doi.org/10.1086/166344
Bankoti, N.S., Joshi, N.C., Pande, B., Pande, S., Uddin, W., and Pandey, K., Asymmetric behavior of different solar activity features over solar cycles 20–23, New Astron., 2011, vol.16, pp. 269–275. https://doi.org/10.1016/j.newast.2010.11.008
Belucz, B., and Dikpati, M., Role of asymmetric meridional circulation in producing north–south asymmetry in a solar cycle dynamo model, Astrophys. J., 2013, vol. 779, p. 4. https://doi.org/10.1088/0004-637X/779/1/4
Carbonell, M., Terradas, J., Oliver, R., and Ballester, J. L., The statistical significance of the North–South asymmetry of solar activity revisited, Astron. Astrophys., 2007, vol. 476, pp. 951–957. https://doi.org/10.1051/0004-6361:20078004
Choudhuri, A.R., The origin of the solar magnetic cycle, Pramana, 2011, vol. 77, no. 1, pp. 77–96. https://doi.org/10.1007/s12043-011-0113-4
Chowdhury, P., Choudhary, D.P., and Gosain, S., A study of the hemispheric asymmetry of sunspot area during solar cycles 23 and 24, Astrophys. J., 2013, vol. 768, p. 188. https://doi.org/10.1088/0004-637X/768/2/188
Deng, L.H., Xiang, Y.Y., Qu, Z.N., and An, J.M., Systematic regularity of hemispheric sunspot areas over the past 140 years, Astron. J., 2016, vol. 151, p. 70. https://doi.org/10.3847/0004-6256/151/3/70
Feldman, U., Doschek, G. A., and Klimchuk, J. A., The occurrence rate of soft X-ray flares as a function of solar activity, Astrophys. J., 1997, vol. 474, p. 511. https://doi.org/10.1086/303428
Garcia, H.A., Evidence for solar-cycle evolution of north–south flare asymmetry during cycles 20 and 21, Sol. Phys., 1990, vol. 127, pp. 185–197. https://doi.org/10.1007/BF00158522
Gnevyshev, M.N. and Ohl, A.I., On the 22-year cycle of solar activity, Astron. Zh., 1948, vol. 25, pp. 18–20.
Goel, A., and Choudhuri, A.R., The hemispheric asymmetry of solar activity during the last century and the solar dynamo, Res. Astron. Astrophys., 2009, vol. 9, pp. 115–126.
Heras, A. M., Sanahuja, B., Shea, M. A., and Smart, D. F., Some comments on the east–west solar flare distribution during the 1976–1985 period, Sol. Phys., 1990, vol. 126, pp. 371–383. https://doi.org/10.1007/BF00153057
Javaraiah, J., North–south asymmetry in small and large sunspot group activity and violation of even–odd solar cycle rule, Astrophys. Space Sci., 2016, vol. 361, p. 208. https://doi.org/10.1007/s10509-016-2797-x
Joshi, A., Asymmetries during the maximum phase of solar cycle 22, Sol. Phys., 1995, vol. 157, pp. 315–324. https://doi.org/10.1007/BF00680624
Joshi, B., and Pant, P., Distribution of Hα flares during solar cycle 23, Astron. Astrophys., 2005, vol. 431, pp. 359–363. https://doi.org/10.1051/0004-6361:20041986
Joshi, B., Pant, P., and Manoharan, P.K., North–south distribution of solar flares during cycle 23, J. Astrophys. Astron., 2006, vol. 27, pp. 151–157. https://doi.org/10.1007/BF02702517
Joshi, B., Bhattacharyya, R., Pandey, K.K., Kushwaha, U., and Moon, Y.J., Evolutionary aspects and north–south asymmetry of soft X-ray flare index during solar cycles 21, 22, and 23, Astron. Astrophys., 2015, vol. 581, pp. 1–11. https://doi.org/10.1051/0004-6361/201526369
Joshi, N.C., Bankoti, N.S., Pande, S., Pande, B., and Pandey, K., Study of distribution and asymmetry of solar active prominences during solar cycle 23, Sol. Phys., 2009, vol. 260, pp. 451–463. https://doi.org/10.1007/s11207-009-9446-2
Joshi, N.C., Bankoti, N.S., Pande, S., Pande, B., Uddin, W., and Pandey, K., Statistical analysis of soft X-ray solar flares during solar cycles 21, 22 and 23, New Astron., 2010, vol. 15, pp. 538–546. https://doi.org/10.1016/j.newast.2010.01.002
Komitov, B., and Bonev, B., Amplitude variations of the 11 year cycle and the current solar maximum 23, Astrophys. J. Lett., 2001, vol. 554, p. L119. https://doi.org/10.1086/320908
Kong, D. F., Qu, Z. N., and Guo, Q. L., The north–south asymmetry of solar filaments separately at low and high latitudes in solar cycle 23, Res. Astron. Astrophys., 2015, vol.15, pp. 77–84. https://doi.org/10.1088/1674-4527/15/1/008
Kramynin, A.P., and Mikhalina, F.A., Latitude–longitude characteristics of the north–south asymmetry of solar activity, Geomagn. Aeron. (Engl. Transl.), 2018, vol. 58, pp. 937–941. https://doi.org/10.1134/S0016793218070125
Letfus, V., and Ruzickova-Topolova, B., Time variation of the EW asymmetry of flare numbers with respect to the phase of solar cycles. Bull. Astron. Inst. Czech., 1980, vol. 31, pp. 232–239.
Li, K.J., Schmieder, B., and Li, Q.S., Statistical analysis of the X-ray flares (M ≥ 1) during the maximum period of solar cycle 22, Astron. Astrophys. Suppl. Ser.,1998, vol. 131, pp. 99–104. https://doi.org/10.1051/aas:1998254
Li, K.J., Wang, J.X., Xiong, S.Y., Liang, H.F., Yun, H.S., and Gu, X.M., Regularity of the north–south asymmetry of solar activity, Astron. Astrophys., 2002, vol. 383, pp. 648–652. https://doi.org/10.1051/0004-6361:20011799
Li, K.J., Liu, X.H., Zhan, L.S., Liang, H.F., Zhao, H.J., and Zhong, S.H., Asymmetry of solar active prominences separately at low and high latitudes from 1957 to 1998, New Astron., 2003, vol. 8, pp. 655–664. https://doi.org/10.1016/S1384-1076(03)00053-8
Li, K.J., Gao, P.X., and Zhan, L.S., The long-term behavior of the north–south asymmetry of sunspot activity, Sol. Phys., 2009a, vol. 254, pp. 145–154. https://doi.org/10.1007/s11207-008-9284-7
Li, K.J., Gao, P.X., Zhan, L.S., Shi, X.J., and Zhu, W.W., The north–south asymmetry of solar activity at high latitudes, Mon. Not. R. Astron. Soc., 2009b, vol. 394, pp. 231–238. https://doi.org/10.1111/j.1365-2966.2008.14172.x
Li, K.J., Chen, H.D., Zhan, L.S., Li, Q.X., Gao, P.X., Mu, J., Shi, X.J., and Zhu, W.W., Asymmetry of solar activity in cycle 23, J. Geophys. Res.: Space Phys., 2009c, vol. 114, p. A04101. https://doi.org/10.1029/2009JA014061
Pandey, K.K., Yellaiah, G., and Hiremath, K.M., Latitudinal distribution of soft X-ray flares and disparity in butterfly diagram, Astrophys. Space Sci., 2015, vol. 356, pp. 215–224. https://doi.org/10.1007/s10509-014-2148-8
Parker, E.N., Hydromagnetic dynamo models, Astrophys. J., 1995, vol. 122, p. 293. https://doi.org/10.1086/146087
Schüssler, M. and Cameron, R.H., Origin of the hemispheric asymmetry of solar activity, Astron. Astrophys., 2018, vol. 618, p. A89. https://doi.org/10.1051/0004-6361/201833532
Shetye, J., Tripathi, D., and Dikpati, M., Observations and modeling of north–south asymmetries using a flux transport dynamo, Astrophys. J., 2015, vol. 799, pp. 220–231. https://doi.org/10.1088/0004-637X/799/2/220
Temmer, M., Veronig, A., Hanslmeier, A., Otruba, W., and Messerotti, M., Statistical analysis of solar H flares, Astron. Astrophys., 2001, vol. 375, pp. 1049–1061. https://doi.org/10.1051/0004-6361:20010908
Verma, V.K., On the distribution and asymmetry of solar active prominences, Sol. Phys., 2000, vol. 194, pp. 87–101. https://doi.org/10.1023/A:1005232619582
Viktorinová, B., and Antalová, A., LDE flares in the 21st solar cycle (1976–1986). I. Comparison of the time occurrences of H-alpha and LDE flares, Bull. Astron. Inst. Czech., 1991, vol. 42, pp. 144–157.
Vizoso, G., and Ballester, J. L., The north–south asymmetry of sunspots, Astron. Astrophys., 1990, vol. 229, pp. 540–546. https://doi.org/10.1051/0004-6361:20078004
ACKNOWLEDGMENTS
We are thankful to the National Geophysical Data Center (NGDC) and its sister data centers merged into the National Centers for Environmental Information (NCEI), NOAA. We sincerely acknowledge the support extended by Jadavpur University, West Bengal India. This work is a part of RUSA 2.0 Faculty Major Research Project under Jadavpur University (Ref: R-11/437/19).
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Amrita Prasad, Roy, S., Panja, S.C. et al. Study of Distribution and Asymmetry in Soft X-ray Flares over Solar Cycles 21–24. Geomagn. Aeron. 62, 288–304 (2022). https://doi.org/10.1134/S0016793222030033
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DOI: https://doi.org/10.1134/S0016793222030033