A Comparison Between Global Proxies of the Sun's Magnetic Activity Cycle: Inferences from Helioseismology (2015)
Attributed to:
Warwick Astrophysics Consolidated Grant 2014-2017
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1507.02854
Publication URI: https://arxiv.org/abs/1507.02854
Type: Other