System Upgrade on Tue, May 28th, 2024 at 2am (EDT)
Existing users will be able to log into the site and access content. However, E-commerce and registration of new users may not be available for up to 12 hours.For online purchase, please visit us again. Contact us at customercare@wspc.com for any enquiries.
Results: 1 - 1of1
Save this search
Please login to be able to save your searches and receive alerts for new content matching your search criteria.
NUMERICAL MODELLING OF THE SIZE AND TEMPERATURE VARIATIONS OF STAR SPOTS AND BRIGHT FACULAE OF MAGNETICALLY ACTIVE STARS FROM THE TRANSIT LIGHT CURVES
Preview AbstractIt is known that small-scale structures in the transit light curves of exoplanets can be used to infer the sizes and temperatures of dark spots or bright faculae of their host stars. Among many factors, the precision depends on the observational statistics, the ratio of the size of the exoplanet to that of the dark (or bright) spot and the cadence used in the light curve measurements. We have developed a numerical code allowing us to explore the effects and limitations of such a method for stars of different spectral types.