Bill Chaplin is an excellent communicator, as his students at University of Birmingham (United Kingdom), where he teaches Solar and Stellar Physics, would certainly attest. In recent years, this data analysis expert has worked on BiSON (Birmingham Solar Oscillations Network), a network of six observatories monitoring low-degree oscillation modes in the Sun. Not long ago, he made the transition from the Sun to other stars and is currently leading a task group working on solar-type stars for the Kepler mission. In this interview he recalls the origins of Helioseismology and clarifies some of
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