Skewness and kurtosis of solar wind proton distribution functions: The normal inverse-Gaussian model and its implications (2024)
Attributed to:
Space and planetary physics 2022-2025
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202347874
Publication URI: https://api.elsevier.com/content/abstract/scopus_id/85184058765
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics