Comparison of the Efficiency of Machine Learning Methods in Studying the Importance of Input Features in the Problem of Forecasting the Dst Geomagnetic Index

Author:

Vladimirov R. D.,Shirokiy V. R.,Myagkova I. N.,Barinov O. G.,Dolenko S. A.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Geophysics

Reference31 articles.

1. Akasofu, S.-I. and Chapman, S., Solar–Terrestrial Physics, Oxford: Clarendon Press, 1972.

2. Amata, E., Pallocchia, G., Consolini, G., et al., Comparison between three algorithms for Dst predictions over the 2003–2005 period, J. Atmos. Sol-Terr. Phys., 70, 496–502 (2008).

3. Barkhatov, N.A., Bellustin, N.S., Levitin. A.E., and Sakharov, S.Y., Comparison of efficiency of artificial neural networks for forecasting the geomagnetic activity index Dst, Radiophys. Quantum Electron., 2000, vol. 43, no. 5, pp. 347–355.

4. Belov, A.V., Villoresi, J., Dorman, L.I., et al., Effect of the space on operation of satellites, Geomagn. Aeron. (Engl. Transl.), 2004, vol. 44, no. 4, pp. 461–468.

5. Artificial neural networks for determining magnetospheric conditions;J. Bortnik,2018

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