The Influence of Eruptive Processes in Active Regions on Oscillations of the Magnetic Field Parameters in Sunspot Umbrae
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Geophysics
Link
https://link.springer.com/content/pdf/10.1134/S0016793223070290.pdf
Reference16 articles.
1. Efremov, V.I., Parfinenko, L.D., Solov’ev, A.A., and Riehokainen, A., Long-period oscillations of sunspot magnetic fields by simultaneous observations of the Global Oscillation Network Group and Solar and Heliospheric Observatory/Michelson Doppler Imager, Geomagn. Aeron. (Engl. Transl.), 2016, vol. 56, no. 7, pp. 897–902.
2. Griñón-Marín, A.B., Pastor Yabar, A., Socas-Navarro, S., et al., Discovery of long-period magnetic field oscillations and motions in isolated sunspots, Astron. Astrophys., 2020, vol. 635, id A64.
3. Li, Y.X., Jing, J., Tan, C.G., et al., The change of magnetic inclination angles associated with the X3.4 flare on December 13, Sci. China Ser. G, 2006, vol. 52, no. 11, pp. 1702–1706.
4. Liu, C., Deng, N., Liu, Y., et al., Rapid change of δ spot structure associated with seven major flares, Astrophys. J., 2005, vol. 622, no. 1, pp. 722–736.
5. Liu, C., Xu, Y., Cao, W., et al., Flare differentially rotates sunspot on Sun’s surface, Nat. Commun., 2016, vol. 7, p. 13104.
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