The iτSBD magnetic braking model attributes the boost K to irradiation-driven winds and the disruption η to a spike in convective turnover time at the fully convective boundary, yielding CV tracks consistent with observations.
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Stellar magnetic cycle variability decreases with faster rotation and higher dynamo number, shown by positive correlation with rotation period and negative correlations with Ro^{-2} and cycle-to-rotation ratio in Mount Wilson data and models.
A joint convective coupling index shows moderate, age-dependent correlation with rotation periods of solar-mass stars, stronger in younger objects and weaker later.
citing papers explorer
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Mechanisms for magnetic braking boost and disruption: the role of irradiation-driven winds and convective turnover time spike in cataclysmic variables
The iτSBD magnetic braking model attributes the boost K to irradiation-driven winds and the disruption η to a spike in convective turnover time at the fully convective boundary, yielding CV tracks consistent with observations.
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Stellar cycle variability in Mount Wilson stars and dynamo models: Rotation rate and dynamo number dependency
Stellar magnetic cycle variability decreases with faster rotation and higher dynamo number, shown by positive correlation with rotation period and negative correlations with Ro^{-2} and cycle-to-rotation ratio in Mount Wilson data and models.
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How plasma coupling and convective-zone depth shape the rotation of solar-mass stars
A joint convective coupling index shows moderate, age-dependent correlation with rotation periods of solar-mass stars, stronger in younger objects and weaker later.