Abstract
We present a study of the frequency of occurrence of quasi-periodic fluctuations (QPFs) of microwave radiation from solar active regions at the pre-flare stage. We used correlation curves obtained with the Nobeyama Radioheliograph (NoRH). We analyzed 529 flares of classes X, M, and C (according to the GOES classification). In a significant number of considered events (approximately 75% of the powerful flares and 50% of the weaker flares), preflare fluctuations of microwave radiation with a duration of up to ten pulses are observed. The character of preflare fluctuations is different in different cases. In some cases, almost harmonic oscillations are observed. In most cases, the fluctuations are sporadic and look like a sequence of weak flares. It is possible that the nature of the preflare QPFs is different in different cases.
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ACKNOWLEDGMENTS
The work was performed using data from the Nobeyama Radioheliograph, the observations on which were 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 authors are grateful to the anonymous referee for useful advice and comments.
Funding
The work was carried out within the framework of the State Assignment (No. 1021032422589-5, Multiwave active Sun,—Study of solar activity, cyclicity, solar-terrestrial relations and solar-stellar analogies on various time scales based on multiwave observations).
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Abramov-Maximov, V.E., Bakunina, I.A. The Frequency of Occurrence of Pre-Flare Fluctuations in Microwave Radiation of Active Regions. Geomagn. Aeron. 63, 916–919 (2023). https://doi.org/10.1134/S0016793223070022
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DOI: https://doi.org/10.1134/S0016793223070022