Quantifying the Difference Between the Flux-Tube Expansion Factor at the Source Surface and at the Alfvén Surface Using a Global MHD Model for the Solar Wind
Crossref DOI link: https://doi.org/10.1007/s11207-015-0739-3
Published Online: 2015-07-29
Published Print: 2015-08
Update policy: https://doi.org/10.1007/springer_crossmark_policy
Cohen, O.
Text and Data Mining valid from 2015-07-29