Stellar Surface Magnetoconvection as a Source of Astrophysical Noise. III. Sun-as-a-Star Simulations and Optimal Noise Diagnostics (2019)
Attributed to:
Queen's University Belfast Consolidated Grant in Solar Physics and Solar System Studies 2017 - 2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/ab16d3
Publication URI: http://dx.doi.org/10.3847/1538-4357/ab16d3
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1
ISSN: 0004-637X