Skewness and kurtosis of solar wind proton distribution functions: The normal inverse-Gaussian model and its implications (2024)
Attributed to:
Solar System Consolidated Grant 2022-25
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202347874
Publication URI: http://dx.doi.org/10.1051/0004-6361/202347874
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics