An analytical model of turbulence in Parker spiral geometry and associated magnetic field line lengths (2022)
Attributed to:
Consolidated Solar and Heliospheric Physics Research at UCLan
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2212.02415
Publication URI: https://arxiv.org/abs/2212.02415
Type: Other