Author:
Strekalova P. V.,Solov’ev A. A.,Smirnova V. V.,Nagovitsyn Yu. A.
Subject
Space and Planetary Science,Geophysics
Reference8 articles.
1. Fontenla, J.M., Curdt, W., Haberreiter, M., Harder, J., and Tian, H., Semiempirical models of the solar atmosphere. III. Set of non-LTE models for far-ultraviolet/extreme-ultraviolet irradiance computation, Astrophys. J., 2009, vol. 707, no. 1, pp. 482–502.
2. Javaherian, M., Safari, H., and Dadashi, N., Statistical properties of photospheric magnetic elements observed by the Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory, Sol. Phys., 2017, vol. 292, no. 11, id 164.
3. Lemen, J.R., Title, A.M., Akin, D.J., et al., The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO), 2012, Sol. Phys., vol. 275, no. 1–2, pp. 17–40.
4. Nita, G.M., Fleishman, G.D., and Gary, D.E., GS-3D simulator: An interactive IDL widget tool for simulating spatially resolved gyrosynchrotron spectra emitted by solar radio bursts, Bull. Am. Astron. Soc., 2009, vol. 41, p. 839.
5. Solov’ev, A.A. and Kirichek, E.A., Analytical model of an asymmetric sunspot with a steady plasma flow in its penumbra, Sol. Phys., 2016, vol. 291, no. 6, pp. 1647–1663.