Stellar Surface Magnetoconvection as a Source of Astrophysical Noise. III. Sun-as-a-Star Simulations and Optimal Noise Diagnostics (2019)
Attributed to:
The transient sky: an integrated programme of study 2011 - 2016
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