The impact of coronal hole characteristics and solar cycle activity in reconstructing coronal holes...
The impact of coronal hole characteristics and solar cycle activity in reconstructing coronal holes with EUHFORIA
About this item
Full title
Author / Creator
Asvestari, E , Heinemann, S G , Temmer, M , Pomoell, J , Kilpua, E , Magdalenic, J and Poedts, S
Publisher
Bristol: IOP Publishing
Journal title
Language
English
Formats
Publication information
Publisher
Bristol: IOP Publishing
Subjects
More information
Scope and Contents
Contents
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...
Alternative Titles
Full title
The impact of coronal hole characteristics and solar cycle activity in reconstructing coronal holes with EUHFORIA
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Author / Creator
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Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2557298974
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2557298974
Other Identifiers
ISSN
1742-6588
E-ISSN
1742-6596
DOI
10.1088/1742-6596/1548/1/012004
