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/10.1007/s11207-015-0728-6
Publication URI: http://dx.doi.org/10.1007/s11207-015-0728-6
Type: Journal Article/Review
Parent Publication: Solar Physics
Issue: 11