Solar Analogs as a Tool to Understand the Sun
Abstract
Solar analogs, broadly defined as stars similar to the Sun in mass or spectral type, provide a useful laboratory for exploring the range of Sun-like behaviors and exploring the physical mechanisms underlying some of the Sun's most elusive processes like coronal heating and the dynamo. We describe a series of heliophysics-motivated, but astrophysics-like studies of solar analogs. We argue for a range of stellar observations, including (a) the identification and fundamental parameter determination of new solar analogs, and (b) characterizing emergent properties like activity, magnetism, and granulation. These parameters should be considered in the framework of statistical studies of the dependences of these observables on fundamental stellar parameters like mass, metallicity, and rotation.
Cite
@article{arxiv.2009.05672,
title = {Solar Analogs as a Tool to Understand the Sun},
author = {Allison Youngblood and Steve Cranmer and Sam Van Kooten and James Paul Mason and J. Sebastian Pineda and Kevin France and Dmitry Vorobiev and Frank Eparvier and Yuta Notsu},
journal= {arXiv preprint arXiv:2009.05672},
year = {2020}
}
Comments
3 pages, 1 table; white paper submitted to the Heliophysics 2050 Workshop