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Cited article:
Yulia Shugay, Vladimir Slemzin, Igor Veselovsky
J. Space Weather Space Clim., 4 (2014) A24
Published online: 2014-08-05
This article has been cited by the following article(s):
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Journal of Geophysical Research: Space Physics 120 (10) 8210 (2015)
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Possible causes of the discrepancy between the predicted and observed parameters of high-speed solar wind streams
Yu. S. Shugay, I. S. Veselovsky, V. A. Slemzin, Yu. I. Yermolaev and D. G. Rodkin
Cosmic Research 55 (1) 20 (2017)
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Prediction of geoeffective solar wind streams near earth according to solar observational data
Yu. S. Shugay, V. A. Slemzin, D. G. Rodkin and I. S. Veselovsky
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Solar Coronal Modeling by Path-conservative HLLEM Riemann Solver
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Magnetic evolution linked to the interrelated activity complexes involving transequatorial coronal holes
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Influence of coronal mass ejections on parameters of high-speed solar wind: a case study
Yulia Shugay, Vladimir Slemzin, Denis Rodkin, Yuri Yermolaev and Igor Veselovsky
Journal of Space Weather and Space Climate 8 A28 (2018)
DOI: 10.1051/swsc/2018015
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Mapping magnetic field lines between the Sun and Earth
B. Li, Iver H. Cairns, J. T. Gosling, G. Steward, M. Francis, D. Neudegg, H. Schulte in den Bäumen, P. R. Player and A. R. Milne
Journal of Geophysical Research: Space Physics 121 (2) 925 (2016)
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Development of Coronal Holes Index For Study of Coronal Hole Geo-Effectiveness
Anwar Santoso, Laode Muhammad Musafar K., Fitri Nuraeni, Visca Wellyanita, Mira Juangsih and Anton Winarko
Journal of Physics: Conference Series 2214 (1) 012025 (2022)
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