1. Alexeeva, I.V. and Kim, I.S., On critical heights and longitudinal magnetic fields strength in prominences, in Nature of Prominences and their role in Space Weather (Proceedings IAU Symp no. 300), Schmieder, B., Malherbe, J.-M. and Wu, S.T., Eds., IAU, 2014, pp. 391–392.
2. Alexeeva, I.V., Bougaenko, O.I., Kim, I.S., Popov, V.V., and Seleznev, D.A., Magnetic field of quiescent prominences of August 11, 1999, in ESA SP-505, 2002, pp. 325–328.
3. Apushkinskii, G.P., Gunder, K., Nesterov, N.S., Nikitin, N.S., Strepka, I.D., Topchilo, N.A., and Tsyganov, A.N., Radio astronomical measurements of magnetic fields in prominences, Astron. Rep., 1996, vol. 40, pp. 393–396.
4. Bogod, V.M. and Gelfreikh, G.B., Measurements of the magnetic field and the gradient of temperature in the solar atmosphere above a flocculus using radio observations, Sol. Phys., 1980, vol. 67, pp. 29–46. doi 10.1007/BF00146680
5. Bommier, V., Sahal-Brechot, S., and Leroy, J.-L., The linear polarization of hydrogen H-beta radiation and the joint diagnostic of magnetic field vector and electron density in quiescent prominences. I. The magnetic field. II. The electron density, Astron. Astrophys., 1986, vol. 156, pp. 79–94.