Forward Modelling of Brightness Variations in Sun-Like Stars. I. Emergence and Surface Transport of Magnetic Flux

Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201833393
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Emergence of Small-Scale Magnetic Flux in the Quiet Sun

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2020English

A Quantitative Study of Magnetic Flux Transport on the Sun

Symposium - International Astronomical Union
1983English

Magnetic Braking of Sun-Like and Low-Mass Stars: Dependence on Coronal Temperature

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Magnetic Flux Transport at the Solar Surface

Space Science Reviews
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

The Sun in Time: Detecting and Modelling Magnetic Inhomogeneities on Solar-Type Stars

International Astronomical Union Colloquium
1994English

What Fraction of Sun‐like Stars Have Planets?

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

Correlations Between Brightness Fields and Magnetic Fields on the Sun

Symposium - International Astronomical Union
1968English

The Chemical Homogeneity of Sun-Like Stars in the Solar Neighborhood

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

An Analytic Theory of Adiabatic P-Modes in the Atmospheres of the Sun and Sun-Like Stars

International Astronomical Union Colloquium
1995English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy