Using Kepler transit observations to measure stellar spot belt migration rates
J. Llama, M. Jardine, D. H. Mackay, R. Fares

TL;DR
This study explores how continuous Kepler transit data can be used to measure the migration rates of stellar spot belts, providing insights into stellar magnetic activity and dynamo processes.
Contribution
It introduces a simulation-based method to recover star spot belt migration rates from transit lightcurves, especially for active stars.
Findings
Spot belt drift rates can be measured for active stars.
Low-activity stars require longer observation periods to detect drift.
Transit lightcurves can reveal magnetic cycle characteristics.
Abstract
Planetary transits provide a unique opportunity to investigate the surface distributions of star spots. Our aim is to determine if, with continuous observation (such as the data that will be provided by the Kepler mission), we can in addition measure the rate of drift of the spot belts. We begin by simulating magnetic cycles suitable for the Sun and more active stars, incorporating both flux emergence and surface transport. This provides the radial magnetic field distribution on the stellar surface as a function of time. We then model the transit of a planet whose orbital axis is misaligned with the stellar rotation axis. Such a planet could occult spots at a range of latitudes. This allows us to complete the forward modelling of the shape of the transit lightcurve. We then attempt the inverse problem of recovering spot locations from the transit alone. From this we determine if transit…
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