Skip to main content
Log in

Oscillations of the Microwave Emission of Solar Active Region 12673 before Flares

  • Published:
Geomagnetism and Aeronomy Aims and scope Submit manuscript

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.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1.
Fig. 2.
Fig. 3.

Similar content being viewed by others

REFERENCES

  1. 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.

    Article  Google Scholar 

  2. 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.

    Article  Google Scholar 

  3. 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.

    Article  Google Scholar 

  4. 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.

    Article  Google Scholar 

  5. 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.

    Google Scholar 

  6. 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.

  7. 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.

    Article  Google Scholar 

  8. 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.

    Google Scholar 

  9. 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.

    Google Scholar 

  10. 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.

    Google Scholar 

  11. 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.

    Article  Google Scholar 

  12. 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.

    Article  Google Scholar 

  13. 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.

  14. 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.

    Article  Google Scholar 

  15. 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.

  16. Nakajima, H., Nishio, M., Enome, S., et al., The Nobeyama Radioheliograph, Proc. IEEE, 1994, vol. 82, pp. 705–713.

    Article  Google Scholar 

  17. 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.

    Article  Google Scholar 

  18. 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.

  19. Torrence, C. and Compo, G.P., A practical guide to wavelet analysis, Bull. Am. Meteorol. Soc., 1998, vol. 79, pp. 61–78.

    Article  Google Scholar 

Download references

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

Authors

Corresponding author

Correspondence to V. E. Abramov-Maximov.

Ethics declarations

The authors declare to have no conflict of interest.

Additional information

Translated by M. Chubarova

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

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

Download citation

  • Received:

  • Revised:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1134/S001679321907003X

Navigation