1. Banin, V.G. and Fedorova, A.S., The strong chromospheric flare of November 5, 1970, in Issledovaniya po geomagnetizmu, aeronomii i fizike Solntsa (Studies on Geomagnetism, Aeronomy, and Solar Physics), Irkutsk: SibIZMIR AN SSSR, 1971, no. 2, pp. 73–85.
2. Hirayama, T., Theoretical model of flares and prominences. I. Evaporating flare model, Sol. Phys., 1974, vol. 34, pp. 323–338.
3. Kichigin, G.N., Miroshnichenko, L.I., Sidorov, V.I., et al., Specific features of the strong solar event of July 23, 2002: the particle acceleration source model, in Trudy vserossiiskoi konferentsii “Solnechnaya i solnechno–zemnaya fizika-2010” (Proceedings of the All-Russian Conference “Solar and Solar–Terrestrial Physics- 2010”), St. Petersburg, 2010, pp. 201–204.
4. Kichigin, G.N., Miroshnichenko, L.I., Sidorov, V.I., et al., Dynamics of accelerated ions in coronal loops and model of a gamma-ray source, Plasma Phys. Rep., 2014, vol. 40, no. 3, pp. 178–193.
5. Kichigin, G.N., Miroshnichenko, L.I., Sidorov, V.I., et al., Diamagnetic reduction in the magnetic field above a sunspot in the gamma-ray burst on July 14, 2000, Plasma Phys. Rep., 2015, vol. 41, no. 8, pp. 651–655.