Abstract
A new mathematical model was proposed using an ordinary differential equation that analytically (when the index of geomagnetic activity Kp = const or Kp ≈ const) or numerically (if Kp(t) ≠ const) describes perpendicular (for a pitch angle of 90°) differential or integral fluxes of relativistic electrons in a geostationary (geosynchronous) orbit, as well as in any circular orbit in the Earth’s magnetosphere. The model assumes that the fluxes depend on the local time LT in orbit, the Kp, McIlwain parameter L and the perpendicular differential flux or integral flux of relativistic electrons taken at 00 LT. We use observations of relativistic (>2 MeV) electron fluxes averaged over the local hour along the orbit of the GOES spacecraft from 1995 to 2009. The model is compared with these data. Almost perfect agreement was obtained for observations with the model, where the prediction efficiency of accuracy of the model at PE = 0.9989. Using similar data from the GOES 10 allows one to obtain PE = 0.9924. The proposed formulas make it possible to find, for example, the average value of the perpendicular integral flux of relativistic electrons per day and to predict the maximum perpendicular integral flux of relativistic electrons in the geostationary orbit approximately 1 day ahead. The nonlinear effect is theoretically predicted in the form of a nonlinear dependence of the ratio of the maximum perpendicular integral flux to the minimum flux of charged particles in the geostationary orbit from the Kp-index of geomagnetic activity. Thus far, comparison of the model has been made with the averaged integral relativistic electron fluxes produced for the 0 ≤ Kp < 6 range with a predicted maximum flux ratio of 24.4139 times at Kp = 8 and with the prediction efficiency of accuracy of the nonlinear effect \(PE\) = 0.8678.
REFERENCES
Baker, D.N., McPherron, R.L., Cayton, T.E., and Kebesadel, R.W., Linear prediction filter analysis of relativistic electron properties at 6.6 RE, J. Geophys. Res.: Space, 1990, vol. 95, no. 9, pp. 15133–15140. https://doi.org/10.1029/JA095iA09p15133
Borovsky, J.E., Friedel, R.H.W., and Denton, M.H., Statistically measuring the amount of pitch angle scattering that energetic electrons undergo as they drift across the plasmaspheric drainage plume at geosynchronous orbit, J. Geophys. Res.: Space, 2014, vol. 119, no. 3, pp. 1814–1826. https://doi.org/10.1002/2013JA019310
Borovsky, J.E., Cayton, T.E., Denton, M.H., Belian, R.D., Christensen, R.A., and Ingraham, J.C., The proton and electron radiation belts at geosynchronous orbit: Statistics and behavior during high-speed stream-driven storms, J. Geophys. Res.: Space, 2016, vol. 121, no. 6, pp. 5449–5488. https://doi.org/10.1002/2016JA022520
Efitorov, A.O., Myagkova, I.N., and Dolenko, S.A., Prediction of maximum daily relativistic electron flux at geostationary orbit by adaptive methods, in Proceedings of the 11th International School and Conference “Problems of Geospace”), Semenov, V.S., Kholeva, M.V., Apatenkov, N.Yu., Bobrov, N.Yu., Kosterov, A.A., Samsonov, N.A., Smirnova, T.V., and Yanovskaya, T.B., Eds., St. Petersburg: VVM, 2016, pp. 206–212.
Fok, M.-C., Horne, R.B., Meredith, N.P., and Glauert, S.A., Radiation belt environment model: Application to space weather nowcasting, J. Geophys. Res.: Space, 2008, vol. 113, no. 3, p. A03S08. https://doi.org/10.1029/2007JA012558
Kalegaev, V., Kaportseva, K., Myagkova, I., Shugay, Yu., Vlasova, N., Barinova, W., Dolenko, S., Eremeev, V., and Shiryaev, A., Medium-term prediction of the fluence of relativistic electrons in geostationary orbit using solar wind streams forecast based on solar observations, Adv. Space Res., 2022, vol. 70. https://doi.org/10.1016/j.asr.2022.08.033
Khazanov, G.V., Gamayunov, K.V., and Jordanova, V.K., Self-consistent model of magnetospheric ring current and electromagnetic ion cyclotron waves: The 2–7 May 1998 storm, J. Geophys. Res., 2003, vol. 108, no. A12, pp. 1419–1436. https://doi.org/10.1029/2003JA009856
Li, X., Variations of 0.7–6.0 MeV electrons at geosynchronous orbit as a function of solar wind, Space Weather, 2004, vol. 2, no. 3, p. S03006. https://doi.org/10.1029/2003SW000017
Li, X., Temerin, M., Baker, D.N., Reeves, G.D., and Larson, D., Quantitative prediction of radiation belt electrons at geostationary orbit based on solar wind measurements, Geophys. Res. Lett., 2001, vol. 28, no. 9, pp. 1887–1890. https://doi.org/10.1029/2000GL012681
Ling, A.G., Ginet, G.P., Hilmer, R.V., and Perry, K.L., A neural network-based geosynchronous relativistic electron flux forecasting model, Space Weather, 2010, vol. 8, no. 9, p. S09003. https://doi.org/10.1029/2010SW000576
Lyatsky, W. and Khazanov, G.V., A predictive model for relativistic electrons at geostationary orbit, Geophys. Res. Lett., 2008, vol. 35, no. 15, p. L15108. https://doi.org/10.1029/2008GL034688
Myagkova, I.N., Shirokii, V.R., Shugai, Yu.S., Barinov, O.G., Vladimirov, R.D., and Dolenko, S.A., Short- and medium-range prediction of relativistic electron flux in the Earth’s outer radiation belt by machine learning methods, Russ. Meteorol. Hydrol., 2021, vol. 46, no. 3, pp. 163–171. https://doi.org/10.3103/S1068373921030043
Nishida, A., Geomagnetic Diagnosis of the Magnetosphere, New York: Springer, 1978.
O’Brien, T.P., SEAES-GEO: A spacecraft environmental anomalies expert system for geosynchronous orbit, Space Weather, 2009, vol. 7, no. 9, p. S09003. https://doi.org/10.1029/2009SW000473
Pinto, V.A., Bortnik, J., Moya, P.S., Lyons, L.R., Sibeck, D.G., Kanekal, S.G., Spence, H.E., and Baker, D.N., Radial response of outer radiation belt relativistic electrons during enhancement events at geostationary orbit, J. Geophys. Res.: Space, 2020, vol. 125, no. 5, p. e2019JA027660. https://doi.org/10.1029/2019JA027660
Smolin, S.V., Pitch angle distribution effect on plasma processes in the nocturnal magnetosphere, Geomagn. Aeron., 1993, vol. 33, no. 5, pp. 17–25.
Smolin, S.V., Modelirovanie pitch-uglovoi diffuzii v magnitosfere Zemli (Modeling Pitch Angle Diffusion in the Earth’s Magnetosphere), Krasnoyarsk: Libra, 1996.
Smolin, S.V., Modeling the pitch angle distribution on the dayside of the Earth’s magnetosphere, Zh. Sib. Fed. Univ.: Ser. Mat. Fiz., 2012, vol. 5, no. 2, pp. 269–275.
Smolin, S.V., Modeling the pitch angle distribution on the nightside of the Earth’s magnetosphere, Geomagn. Aeron. (Engl. Transl.), 2015, vol. 55, no. 2, pp. 166–173. https://doi.org/10.1134/S0016793215020152
Smolin, S.V., Simulation of the flux of relativistic electrons in a geostationary orbit in the Earth’s magnetosphere, Prostranstvo, Vremya Fundam. Vzaimodeistviya, 2018a, no. 2, pp. 75–85. https://doi.org/10.17238/issn2226-8812.2018.2.75-85
Smolin, S.V., A simple analytical description for the flux of relativistic (>2 MeV) electrons in a geosynchronous orbit, in Materialy 12-oi Mezhdunarodnoi shkoly-konferentsii “Problemy geokosmosa” (Proceedings of the 12th International School and Conference “Problems of Geospace”), Bobrov, N.Yu., Zolotova, N.V., Kosterov, A.A., and Yanovskaya, T.B., Eds., St. Petersburg: VVM, 2018b, pp. 372–378.
Smolin, S.V., Analytical description of the proton flux of the Earth’s ring current for a pitch angle of 90 degrees, Prostranstvo, Vremya Fundam. Vzaimodeistviya, 2019, no. 2, pp. 70–74. https://doi.org/10.17238/issn2226-8812.2019.2.70-74
Smolin, S.V., Ring current proton dynamics driven by wave-particle interactions during a nonstorm period, J. Sib. Fed. Univ.: Ser. Math. Phys., 2021, vol. 14, no. 1, pp. 98–104. https://doi.org/10.17516/1997-1397-2021-14-1-98-104
Su, Y.-J., Quinn, J.M., Johnston, W.R., McCollough, J.P., and Starks, M.J., Specification of >2 MeV electron flux as a function of local time and geomagnetic activity at geosynchronous orbit, Space Weather, 2014, vol. 12, no. 7, pp. 470–486. https://doi.org/10.1002/2014SW001069
Turner, D.L. and Li, X., Quantitative forecast of relativistic electron flux at geosynchronous orbit based on low-energy electron flux, Space Weather, 2008, vol. 6, no. 5, p. S05005. https://doi.org/10.1029/2007SW000354
Turner, D.L., Li, X., Burin de Roziers, E., and Monk, S., An improved forecast system for relativistic electrons at geosynchronous orbit, Space Weather, 2011, vol. 9, no. 6, p. S06003. https://doi.org/10.1029/2010SW000647
Ukhorskiy, A.Y., Sitnov, M.I., Sharma, A.S., Anderson, B.J., Ohtani, S., and Lui, A.T.Y., Data-derived forecasting model for relativistic electron intensity at geosynchronous orbit, Geophys. Res. Lett., 2004, vol. 31, no. 9, p. L09806. https://doi.org/10.1029/2004GL019616
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Smolin, S.V. A Nonlinear Dependence on the Geomagnetic Activity of the Ratio of the Maximum Flux of Charged Particles in a Geostationary Orbit to the Minimum Flux. Geomagn. Aeron. 63, 574–583 (2023). https://doi.org/10.1134/S0016793223600534
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DOI: https://doi.org/10.1134/S0016793223600534