Abstract
We present a study of quasi-periodic pulsations in the microwave emission from solar active region (AR) NOAA 12673, which produced the strongest flares of the 24th solar activity cycle. The data from daily observations of the Sun at the Nobeyama Radioheliograph at a frequency of 17 GHz were used. The microwave emission of the AR was analyzed for September 3–4, 2017, i.e., before the first M-class flare, which occurred on September 4. Long-period pulsations in the microwave emission with periods of approximately 100 min appeared at least 7 h before the first M-class flare, which was followed by strong flare activity in NOAA 12673. The effect is similar to the previously discovered preflare oscillatory phenomena with different periods manifested in different ranges.
Similar content being viewed by others
REFERENCES
Abramov-Maximov, V.E., Gelfreikh, G.B., and Shibasaki, K., Quasi-periodic oscillations of solar active regions in connection with their flare activity—NoRH observations, Sol. Phys., 2011, vol. 273, pp. 403–412.
Abramov-Maximov, V.E. and Bakunina, I.A., Features of short-period oscillations of microwave emission from the solar active region before the flare, Phys. At. Nucl., 2018, vol. 81, no. 3, pp. 379–383.
Aleshin, V.I., Kobrin, M.M., and Korshunov, A.I., Quasiperiodic components with periods of from 30 to 60 min in the fluctuation spectra of solar radio emission at the 3 cm wavelength, Radiophys. Quantum Electron., 1973, vol. 16, no. 5, pp. 571–576.
Arbuzov, S.I., Flare-associated variations in the spectral slope of radio emission (λ≈3 cm) from solar active regions, Radiophys. Quantum Electron., 1980, vol. 22, no. 10, pp. 803–811.
Avdyushin, S.I., Bogomolov, A.F., Borisova, E.A., et al., Relationship between solar activity and the radio-emission characteristics of solar active regions, Dokl. Akad. Nauk SSSR, 1985, vol. 283, no. 1, pp. 67–70.
Aver’yanikhina, E., Paupere, M., Ozolins, G., and Eliass, M., On the character of amplitude change of intensity fluctuations of solar radio radiation in the decimeter band before powerful radio bursts which are connected with flares, Issled. Soln. Krasnykh Zvezd, 1982, no. 16, pp. 61–74.
Berulis, I.I., Molchanov, A.P., Olyanyuk, V.P., Pogodin, I.E., Pudov, O.Ya., Franchuk, N.G., and Yasnov, L.V., The spectral index and fluctuations of solar radioemission at the λ≈3 cm wavelength, Radiophys. Quantum Electron., 1973, vol. 16, no. 9, pp. 1047–1049.
Berulis, I.I., Kozlovskii, A.L., Losovskii, B.Y., Franchuk, N.G., and Yasnov, L.V., Fluctuations of the radio emission of local sources on the sun based on observations on the RT-22 radio telescope of the Lebedev Institute, Sov. Astron., 1983, vol. 27, no. 5, pp. 563–567.
Borovik, V.N., Abramov-Maximov, V.E., Tlatov, A.G., Opeikina, L.V., Shramko, A.D., and Yasnov, L.V., Signs of preparation of powerful solar flares in September 2017 in microwave radiation and structure of the magnetic field of active region using RATAN-600 and SDO/HMI data, Izv. Krym. Astron. Obs., 2018, vol. 114, no. 1, pp. 89–94.
Durasova, M.S., Kobrin, M.M., and Yudin, O.I., Evidence of quasi-periodic movements in the solar chromosphere and corona, Nature, 1971, vol. 229, no. 3, pp. 82–84.
Gelfreikh, G.B., Grechnev, V.V., Kosugi, T., and Shibasaki, K., Detection of periodic oscillations in sunspot-associated radio sources, Sol. Phys., 1999, vol. 185, pp. 177–191.
Gelfreikh, G.B., Nagovitsyn, Yu.A., and Nagovitsyna, E.Yu., Quasi-periodic oscillations of microwave emission in solar active regions, Publ. Astron. Soc. Jpn., 2006, vol. 58, pp. 29–35.
Kobrin, M.M., Korshunov, A.I., Snegirev, S.D., and Timofeev, B.V., On a sharp increase of quasi-periodic components of fluctuations of inclination of the spectrum of solar radio emission at lambda = 3 cm before active events in August 1972, Soln. Dannye, 1973a, no. 10, pp. 79–85.
Kobrin, M.M., Pakhomov, V.V., Durasova, M.S., et al., Fluctuations of solar radioemission at the 3-cm wavelength using two radiotelescopes that are spaced 1500 km apart, Radiophys. Quantum Electron., 1973b, vol. 16, no. 9, pp. 1036–1039.
Kobrin, M.M., Semenova, S.V., Pahomov, V.V., et al., The study of the phenomenon of the growth of solar centimeter-band radioemission before intense flares, Astron. Tsirk., 1981, no. 1201, pp. 1–3.
Nakajima, H., Nishio, M., Enome, S., et al., The Nobeyama Radioheliograph, Proc. IEEE, 1994, vol. 82, pp. 705–713.
Sych, R., Nakariakov, V.M., Karlicky, M., and Anfinogentov, S., Relationship between wave processes in sunspots and quasi-periodic pulsations in active region flares, Astron. Astrophys., 2009, vol. 505, pp. 791–799.
Tan, B., Yu, Z., Huang, J., Tan, C., and Zhang, Y., Very long-period pulsations before the onset of solar flares, Astrophys. J., 2016, vol. 83, no. 2, id 206.
Torrence, C. and Compo, G.P., A practical guide to wavelet analysis, Bull. Am. Meteorol. Soc., 1998, vol. 79, pp. 61–78.
ACKNOWLEDGMENTS
The study used data from the Nobeyama Radioheliograph, the observations at which are carried out with the support of the International Consortium for the Continued Operation of Nobeyama Radioheliograph, ICCON). ICCON consists of ISEE/Nagoya University, NAOC, KASI, NICT, and GSFC/NASA. The wavelet analysis software was developed by C. Torrence and G. Compo and is available at http://paos.colorado.edu/research/wavelets/. The SWPC PRF data are available at ftp://ftp.ngdc.noaa.gov/STP/ swpc_products/weekly_reports/PRFs_of_SGD/2017/09/. The authors would like to thank I.V. Zimovets for helpful comments.
Funding
The study was performed as part of the State Assignment (subject 0041-2019-0019) with partial support from the RAS Program of basic research 12 “Problems of Origin and Evolution of the Universe.”
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
The authors declare to have no conflict of interest.
Additional information
Translated by M. Chubarova
Rights and permissions
About this article
Cite this article
Abramov-Maximov, V.E., Bakunina, I.A. Oscillations of the Microwave Emission of Solar Active Region 12673 before Flares. Geomagn. Aeron. 59, 822–826 (2019). https://doi.org/10.1134/S001679321907003X
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S001679321907003X