Interchange reconnection as the source of the fast solar wind within coronal holes
Interchange reconnection as the source of the fast solar wind within coronal holes
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Publisher
London: Nature Publishing Group UK
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Language
English
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Publisher
London: Nature Publishing Group UK
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Scope and Contents
Contents
The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called ‘coronal holes’. The energy source responsible for accelerating the plasma is widely debated; however, there is evidence that it is ultimately magnetic in nature, with candidate mechanisms including wave heating
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Full title
Interchange reconnection as the source of the fast solar wind within coronal holes
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TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_10247371
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_10247371
Other Identifiers
ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/s41586-023-05955-3
