Identification of coronal sources of the solar wind from solar images in the EUV spectral range
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Astronomy and Astrophysics,Aerospace Engineering
Link
http://link.springer.com/content/pdf/10.1134/S0010952515010074.pdf
Reference49 articles.
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3. Eselevich, V.G., Fainshtein, V.G., Rudenko, G.V., et al., Forecasting the velocity of quasi-stationary solar wind and the intensity of geomagnetic disturbances produced by it, Cosmic Research, 2009, vol. 47, no. 2 pp. 95–113.
4. McComas, D.J., Bame, S.J., Barker, P., et al., Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer, Space Sci. Rev., 1998, vol. 86, p. 563.
5. Gloecker, G., Cain, J., Ipavich, F.M., et al., Investigation of the composition of solar and interstellar matter using solar wind and pickup ion measurements with SWICS and SWIMS on the ACE spacecraft, Space Sci. Rev., 1998, vol. 86, p. 497.
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