Якутск, Россия
The paper studies the influence of interplanetary factors on the degree of symmetry of the magnetospheric ring current. The geomagnetic indices SYM-H, ASY-H, and interplanetary parameters for the period 1981–2015 are considered. The indicator of the degree of symmetry of the ring current is the ratio SYM-H/ASY-H. Analysis is based on annual averages of geomagnetic and interplanetary parameters. This approach allows us to identify large-scale patterns. The relationships are examined of the degree of symmetry of the ring current and the indices SYM-H and ASY-H with the value B of the interplanetary magnetic field (IMF), the IMF north-south component Bn, and the solar wind velocity V. It is concluded that properties of magnetospheric ring currents are described by these indices more adequately when offsets in their values are taken into account than without regard for them. It is found that when offsets in ASY-H are considered the symmetric ring current prevails approximately twice over the asymmetric one for average conditions in the solar wind: V<550 km/s, B<10 nT, ǀBnǀ<2 nT. Under quiet solar wind conditions (V<450 km/s, B<5.5 nT, ǀBnǀ<0.7 nT), the degree of symmetry of the ring current increases. It is established that with intensification of interplanetary parameters (V, B, ǀBnǀ) the symmetric ring current index SYM-H grows more strongly than the asymmetric ring current index ASY-H.
geomagnetic indices SYM-H and ASY-H, magnetospheric ring current, interplanetary parameters
1. Alexeev I.I., Belenkaya E.S., Kalegaev V.V., Feldstein Y.I., Grafe A. Magnetic storms and magnetotail currents. J. Geophys. Res. 1996, vol. 101, no. A4, pp. 7737–7747. DOI:https://doi.org/10.1029/95JA03509.
2. Bakhmina K.Yu., Kalegaev V.V. Modeling the partial ring current effect in a disturbed magnetosphere. Geomagnetism and Aeronomy. 2008, vol. 48, no. 6, pp. 713–718.
3. Barkhatov N.A., Levitin A.E., Tserkovnyuk O.M. Relation of the indices characterizing the symmetric (SYM) and asymmetric (ASY) ring currents to the AE (AU, AL) indices of auroral electrojet activity. Geomagnetism and Aeronomy, 2008, vol. 48, no. 4, pp. 499–503.
4. Bhaskar A., Vichare G. Forecasting of SYM-H and ASY-H indices for geomagnetic storms of solar cycle 24 including St. Patricks day, 2015 storm using NARX neural network. Journal of Space Weather and Space Climate. 2019, vol. 9, no. A12. DOI:https://doi.org/10.1051/swsc/2019007.
5. Boroyev R.N., Vasiliev M.S. Relationship of the ASY-H index with interplanetary medium parameters and auroral activity in magnetic storm main phases during CIR and ICME events. Sol.-Terr. Phys. 2020, vol. 6, iss. 1, pp. 35–40. DOI:https://doi.org/10.12737/stp-61202004.
6. Haiducek J.D., Welling D.T., Ganushkina N.Y., Morley S.K., Dogacan Su Ozturk. SWMF global magnetosphere simulations of January 2005: Geomagnetic indices and cross-polar cap potential. Space Weather. 2017, vol. 15, pp. 1567–1587.
7. Hakkinen L.V.T., Pulkkinen T.I., Pirjola R.J., Nevanlinna H., Tanskanen E.I., Turner N.E. Seasonal and diurnal variation of geomagnetic activity: Revised Dst versus external drivers. J. Geophys. Res. 2003, vol. 108, no. A2, p. 1060. DOI:https://doi.org/10.1029/2002JA009428.
8. Iyemori T., Araki T., Kamei T., Takeda M. Mid-latitude geomagnetic indices ASY and SYM (Provisional) No. 1: 1989–1990. Data Analysis Center for Geomagnetism and Space Magnetism; Kyoto University, Japan, 1992, 240 р.
9. Iyemori T., Takeda M., Nose M., et al. Mid-latitude geomagnetic indices ASY and SYM for 2009 (Provisional). Data Analysis Center for Geomagnetism and Space Magnetism; Kyoto University, Japan, 2010. URL: http://wdc.kugi.kyoto-u.ac.jp/aeasy/asy.pdf (accessed October 5, 2021).
10. Kalegaev V.V., Bakhmina K.Yu., Alexeev I.I., Belenkaya E.S., Feldstein Ya.I., Ganushkina N.V. Ring current asymmetry during a magnetic storm.Geomagnetism and Aeronomy. 2008, vol. 48, no. 6, pp. 747–759.
11. Makarov G.A. Geometric factor in seasonal variations of daily average values of the geomagnetic index Dst. Sol.-Terr. Phys. 2020, vol. 6, iss. 4, pp. 50–56. DOI:https://doi.org/10.12737/stp-64202008.
12. Makarov G.A. Offset in the geomagnetic indices of the magnetospheric ring current. Sol.-Terr. Phys. 2021, vol. 7, iss. 3, pp. 29–35. DOI:https://doi.org/10.12737/stp-73202103.
13. Makarov G.A. Geomagnetic indices ASY-H and SYM-H and their relation to interplanetary parameters. Sol.-Terr. Phys. 2022, vol. 8, iss. 4, pp. 36–43. DOI:https://doi.org/10.12737/stp-84202203.
14. Makarov G.A. Large-scale relationships of the geomagnetic indices SYM-H and ASY-H with the north-south IMF component and the solar wind beta parameter. Sol.-Terr. Phys. 2024, vol. 10, iss. 3, pp. 91–96. DOI:https://doi.org/10.12737/stp-103202411.
15. Maltsev Y.P., Arykov A.A., Belova E.G., Gvozdevsky B.B., Safargaleev V.V. Magnetic flux redistribution in the storm time magnetosphere. J. Geophys. Res. 1996, vol. 101, no. A4, pp. 7697–7704.
16. Namuun B., Tsegmed B., Li L.Y., Leghari G.M. Differences in the response to CME and CIR drivers of geomagnetic disturbances. Sol.-Terr. Phys. 2023, vol. 9, iss. 2, pp. 31–36. DOI:https://doi.org/10.12737/stp-92202304.
17. Shi Y., Zesta E., Lyons L.R., Yumoto K., Kitamura K. Statistical study of effect of solar wind dynamic pressure enhancements on dawn-to-dusk ring current asymmetry. J. Geophys. Res. 2006, vol. 111, A10216. DOI:https://doi.org/10.1029/2005JA011532.
18. Singh A.K., Sinha A.K., Pathan B.M., Rajaram R., Rawat R. Effect of prompt penetration on the low latitude ASY indices. J. Atmos. Solar-Terr. Phys. 2013, vol. 94, pp. 34–40.
19. Takalo J., Mursula K. A model for the diurnal universal time variation of the Dst index, J. Geophys. Res. 2001, vol. 106, no. A6, pp. 10905–10914.
20. Tsyganenko N.A., Sitnov M.I. Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms. J. Geophys. Res. 2005, vol. 110, A03208. DOI:https://doi.org/10.1029/2004JA010798.
21. Weygand J.M., McPherron R.L. Dependence of ring current asymmetry on storm phase. J. Geophys. Res. 2006, vol. 111, A11221. DOI:https://doi.org/10.1029/2006JA011808.
22. Zhao M.X., Le G.M., Lu J.Y. Can we estimate the intensities of great geomagnetic storms (ΔSYM-H≤–200 nT) with the Burton equation or the O’Brien and McPherron equation? Astrophys. J. 2022, vol. 928, p. 18. DOI:https://doi.org/10.3847/1538-4357/ac50a8.
23. URL: https://wdc.kugi.kyoto-u.ac.jp/index.html (accessed March 29, 2025).
24. URL: http://omniweb.gsfc.nasa.gov/



