TY  -  
T1  - The impact of coronal hole characteristics and solar cycle activity in reconstructing coronal holes with EUHFORIA 
SN  -  /  
UR  - http://hdl.handle.net/10138/319445 
T3  - Journal of Physics Conference Series 
A1  - Asvestari, E.; Heinemann, S. G.; Temmer, M.; Pomoell, J.; Kilpua, E.; Magdalenic, J.; Poedts, S. 
A2  -  
PB  - IOP Publishing 
Y1  - 2020 
LA  - eng 
AB  - Modelling with high accuracy the open magnetic field and the fast solar wind in the heliosphere is essential for space weather forecasting purposes. Primary sources of open magnetic field flux are Coronal Holes (CH), uni-polar regions that appear as dark patches in the solar corona when observed in X-ray and extreme-ultraviolet (EUV) images due to having significantly lower density and temperature to their surroundings. Therefore, when assessing how well the open magnetic field and the fast sola... 
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KW  - TIME; 115 Astronomy, Space science; 114 Physical sciences 
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