Abstract
Based on an analysis of data for February–March 2023, the report considers the results of studies of the relationship between the occurrence of sporadic microwave radiation preceding the phenomena of coronal mass ejections and these phenomena. The aim is to develop methods for short-term prediction of coronal mass ejections from radio data.
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REFERENCES
Gopalswamy, N., The Sun and space weather, Atmosphere, 2022, vol. 13, no. 11, p. 1781. https://doi.org/10.3390/atmos13111781
Pulkkinen, A., Bernabeu, E., Thomson, A., et al., Geomagnetically induced currents: Science, engineering, and applications readiness, Space Weather, 2017, vol. 15, no. 7, pp. 828–856. https://doi.org/10.1002/2016SW001501
Kutiev, I., Tsagouri, I., Perrone, L., et al., Solar activity impact on the Earth’s upper atmosphere, J. Space Weather Space Clim., 2013, vol. 3, no. A06. https://doi.org/10.1051/swsc/2013028
Tsagouri, I., Galkin, I., and Asikainen, T., Long-term changes in space weather effects on the Earth’s ionosphere, Adv. Space Res., 2017, vol. 59, no. 1, pp. 351–365. https://doi.org/10.1016/j.asr.2016.10.004
Breus, T.K., Binhi, V.N., and Petrukovich, A.A., Magnetic factor in solar-terrestrial relations and its impact on the human body: Physical problems and prospects for research, Usp. Phys., 2016, vol. 59, pp. 502–510. https://doi.org/10.3367/UFNe.2015.12.037693
Vourlidas, A., Improving the medium-term forecasting of space weather: A big picture review from a solar observer’s perspective, Front. Astron. Space Sci., 2021, vol. 8, p. 651527. https://doi.org/10.3389/fspas.2021.651527
Falconer, D.A., Moore, R.I., and Gary, G.A., Magnetogram measures of total nonpotentiality for prediction of solar coronal mass ejections from active regions of any degree of magnetic complexity, Astrophys. J., 2008, vol. 689, pp. 1433–1442. https://doi.org/10.1086/591045
Qahwaji, R., Colak, T., Al-Omari, M., et al., Automated prediction of CMEs using machine learning of CME–flare associations, Sol. Phys., 2008, vol. 248, no. 2, pp. 471–483. https://doi.org/10.1007/s11207-007-9108-1
Al-Omari, M., Qahwaji, R., Colak, T., et al., Machine leaning-based investigation of the associations between CMEs and filaments, Sol. Phys., 2010, vol. 262, no. 2, pp. 511–539. https://doi.org/10.1007/s11207-010-9516-5
Baker, D., van Driel-Gesztelyi, L., and Green, L.M., Forecasting a CME by spectroscopic precursor?, Sol. Phys., 2012, vol. 276, pp. 219–239. https://doi.org/10.1007/s11207-011-9893-4
Chen, P.F., Coronal mass ejections: Models and their observational basis, Liv. Rev. Sol. Phys., 2011, vol. 8, no. 1. https://doi.org/10.12942/lrsp-2011-1
Schmieder, B. and Aulanier, G., What are the physical mechanisms of eruptions and CMEs?, Adv. Space Res., 2011, vol. 49, no. 11, pp. 1598–1606. https://doi.org/10.1016/j.asr.2011.10.023
Green, L.M., Török, T., Vršnak, B., et al., The origin, early evolution and predictability of solar eruptions, Space Sci. Rev., 2018, vol. 214, no. 1, p. 46. https://doi.org/10.1007/s11214-017-0462-5
Casini, R., White, S.M., and Judge, P.G., Magnetic diagnostics of the solar corona: Synthesizing optical and radio techniques, Space Sci. Rev., 2017, vol. 210, pp. 145–181. https://doi.org/10.1007/s11214-017-0400-6
Zheleznyakov, V.V., Radioizluchenie Solntsa i planet (Radio Emission from the Sun and Planets), Moscow: Nauka, 1964.
Zlotnik, E.Ya., Theory of the slowly changing component of solar radio emission. I, Sov. Astron., 1968, vol. 12, no. 2, p. 245.
Zlotnik, E.Ya., The theory of the slowly changing component of solar radio emission. II, Sov. Astron., 1968, vol. 12, no. 3, p. 464.
Kuroda, N., Fleishman, G.D., Gary, D.E., et al., Evolution of flare-accelerated electrons quantified by spatially resolved analysis, Front. Astron. Space Sci., 2020, vol. 7, p. 22. https://doi.org/10.3389/fspas.2020.00022
Nindos, A., Incoherent solar radio emission, Front. Astron. Space Sci., 2020, vol. 7, p. 57. https://doi.org/10.3389/fspas.2020.00057
Vourlidas, A., Radio observations of coronal mass ejection, in Solar and Space Weather Radiophysics: Current Status and Future Developments, Gary, D.E. and Keller, C.U., Eds., Dordrecht: Kluwer Academic Publishers, 2004, vol. 314, pp. 223–242.https://doi.org/10.1007/1-4020-2814-8_11
Vourlidas, A., Carley, E.P., and Vilmer, N., Radio observations of coronal mass ejections: Space weather aspects, Front. Astron. Space Sci., 2020, vol. 7, p. 43. https://doi.org/10.3389/fspas.2020.00043
Carley, E.P., Vilmer, N., and Vourlidas, A., Radio observations of coronal mass ejection initiation and development in the low solar corona, Front. Astron. Space Sci., 2020, vol. 7, p. 551558. https://doi.org/10.3389/fspas.2020.551558
Pohjolainen, S., Vilmer, N., Khan, J.I., et al., Early signatures of large-scale field line opening. Multi-wavelength analysis of features connected with a “halo” CME event, Astron. Astrophys., 2005, vol. 434, pp. 329–341. https://doi.org/10.1051/0004-6361:20041378
Aurass, H., Holman, G., Braune, S., et al., Radio evidence for breakout reconnection in solar eruptive events, Astron. Astrophys., 2013, vol. 555, no. A40. https://doi.org/10.1051/0004-6361/201321111
Aurass, H., Vourlidas, A., Andrews, M.D., et al., Nonthermal radio signatures of coronal disturbances with and without coronal mass ejections, Astrophys. J., 1999, vol. 511, pp. 451–465. https://doi.org/10.1086/306653
Pick, M., Malherbe, J.-M., Kerdraon, A., et al., On the disk Hα and radio observations of the 2003 October 28 flare and coronal mass ejection event, Astrophys. J. Lett., 2005, vol. 631, p. L97. https://doi.org/10.1086/497137
Kobrin, M., Semenova, S.V., Pakhomov, V.V., et al., Results of studies of the effect of increasing long-period pulsations of centimeter radio emission from the Sun before powerful flares, ATs, 1981, no. 1201, pp. 1–3.
Avdyushin, S.I., Bogomolov, A.F., Borisova, E.A., et al., On the connection between solar flare activity and the characteristics of radio emission from local sources on the Sun, Dokl. Akad. Nauk SSSR, 1985, vol. 283, no. 1, pp. 67–70.
Liu, Y. and Zheng, L., Solar microwave radiation flux and the short-term prediction of proton events, in Proc. Solar-Terrestrial Prediction-V (STPW’96), Japan, January 23–27, 1996, Tokyo: RCW, 1997, pp. 196–199.
Li, X.-C. and Kang, L.-Sh., Evidence for a strong correlation of solar proton events with solar radio bursts, Chin. J. Astron. Astrophys., 2005, vol. 5, no. 1, pp. 110–116.
Snegirev, S.D., Fridman, V.M., and Sheiner, O.A., RF Patent 2009136134/28, Byull. Izobret., 2011, no. 15.
Durasova, M.S., Podstrigach, T.S., Fridman, V.M., et al., A study of preflare situations using spectral data on fluxes of solar radio emission in the period from 1970 to 1994, Radiophys. Quantum Electron., 1996, vol. 39, pp. 950–956.
Wang, H., Liu, Ch., Ahn, K., et al., High-resolution observations of flare precursors in the low solar atmosphere, Nat. Astron., 2017, vol. 1, p. 0085. https://doi.org/10.1038/s41550-017-0085
Sheiner, O.A. and Durasova, M.S., Solar microwave precursors and coronal mass ejection: Possible connection, Radiophys. Quantum Electron., 1994, vol. 37, no. 7, pp. 575–578. https://doi.org/10.1007/BF01046806
Sheiner, O.A. and Fridman, V.M., Solar microwave emission phenomena observed during the formation and initial propagation of coronal mass ejections, Radiophys. Quantum Electron., 2010, vol. 53, pp. 281–296.
Sheiner, O.A. and Fridman, V.M., The features of microwave solar radiation observed in the stage of formation and initial propagation of geoeffective coronal mass ejections, Radiophys. Quantum Electron., 2012, vol. 54, pp. 655–666.
Fridman, V.M. and Sheiner, O.A., RF Patent 2630535, 2017.
Vapnik, V.N., Vosstanovlenie zavisimostei po empiricheskim dannym (Recovering Dependencies Based on Empirical Data), Moscow: Nauka, 1979.
Solar-Geophysical Data (explanation of data reports). 1981. Suppl. Iss. 438. ftp//ftp.ngdc.noaa.gov/stp/solardata/solarradio/bursts/radio.txt.
Durasova, M.S., Tikhomirov, Yu.V., and Fridman, V.M., On the frequency distribution of microwave radio bursts during periods associated with the existence of coronal mass ejections, in Aktual’nye problemy fiziki solnechnoi i zvezdnoi aktivnosti. Konf. stran SNG i Pribaltiki (Current Problems in the Physics of Solar and Stellar Activity. Conf. CIS and Baltic Countries), Nizhny Novgorod, June 2–7, 2003, vol. 1, pp. 136–139.
Yan, J., Wu, J., Wu, L., et al., A super radio camera with a one-kilometre lens, Nat. Astron., 2023, vol. 7, p. 750. https://doi.org/10.1038/s41550-023-01932-y
Altyntsev, A., Siberian Radioheliograph: Multi-wave monitoring in the range of 3–12 GHz in February–March 2023, in Tezisy dokl. Konf. “Problemy kosmofiziki” imeni M.I. Panasyuka (Proc. Conf. “Problems of Cosmophysics” Named after M.I. Panasyuk), 2023.
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The study was carried out under project FSWR-2023-0038 within a basic part of a state order of the Ministry of Science and Higher Education of the Russian Federation.
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Translated by M. Chubarova
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Sheiner, O.A., Fridman, V.M. CME Radio Precursors Recorded in February–March 2023. Cosmic Res 62, 210–219 (2024). https://doi.org/10.1134/S0010952523600348
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DOI: https://doi.org/10.1134/S0010952523600348