Influence of coronal mass ejections on parameters of high-speed solar wind: a case study

We investigate the case of disagreement between predicted and observed in-situ parameters of the recurrent high-speed solar wind streams (HSSs) existing for Carrington rotation (CR) 2118 (December 2011) in comparison with CRs 2117 and 2119. The HSSs originated at the Sun from a recurrent polar coron...

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Hlavní autoři:	Shugay Yulia, Slemzin Vladimir, Rodkin Denis, Yermolaev Yuri, Veselovsky Igor
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	EDP Sciences 2018-01-01
Edice:	Journal of Space Weather and Space Climate
Témata:	solar wind prediction models high-speed solar wind streams coronal holes coronal mass ejections interplanetary coronal mass ejections HSS-CME interaction
On-line přístup:	https://doi.org/10.1051/swsc/2018015
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