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Resolving the Radio Photospheres of Main Sequence Stars

Published onMay 31, 2019
Resolving the Radio Photospheres of Main Sequence Stars
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Abstract

We discuss the need for spatially resolved observations of the radio photospheres of main sequence stars. Such studies are fundamental to determining the structure of stars in the key transition region from the cooler optical photosphere to the hot chromosphere — the regions powering exo-space weather phenomena.

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