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Several automated optical telescopes have been setup at appropriate longitudes around the globe to study earthshine variations
and asteroseismology. The first telescope has been setup at Teide Observatory, Tenerife, Spain in October 2004. The intensity
of earthshine relates to the average of Earth’s albedo, and in turn relates to the global temperature of the Earth. A global
network is necessary because each site can measure the earthshine reflected from only a part of the Earth. The network will
also be used for asteroseismology study. It can measure photometric variations of pulsating stars. The long-term and continuous
measurements allow the accurate determination of mode frequencies of stellar pulsations, which provides information on the
properties of stellar interior. 相似文献
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S. Hekker 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The space-borne observatories CoRoT (Convection Rotation and planetary Transits) and Kepler have provided photometric time series data of unprecedented precision for large numbers of stars. These data have revolutionized the fields of transiting exoplanets and asteroseismology. In this review some important asteroseismic results obtained using data from the CoRoT and Kepler space missions concerning stars that show solar-like oscillations are discussed. These results comprise, among others, measurements of the location of the base of the convection zone and helium second-ionization zone in main-sequence stars, the presence (or not) of core-helium burning in red-giant stars, as well as differential rotation in these stars. 相似文献
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