Stellar Surface Magneto-Convection 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/10.48550/arxiv.1903.08446
Publication URI: https://arxiv.org/abs/1903.08446
Type: Other