Highly structured slow solar wind emerging from an equatorial coronal hole (2019)
Attributed to:
Turbulent Heating of Space Plasmas
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1038/s41586-019-1818-7
PubMed Identifier: 31802007
Publication URI: http://europepmc.org/abstract/MED/31802007
Type: Journal Article/Review
Parent Publication: Nature
Issue: 7786
ISSN: 0028-0836