Full-disk helioseismology in the Antarctic

Abstract
The South Pole has been an important site for unimaged helioseismology since 1979. With the rapid development of helioseismology, observations have evolved toward international network and space projects. Future observations from the South Pole will have an important role in validating data from low‐latitude networks, obtained certain measurements comparable only to those made in space and for imaged disk data. The utility of the South Pole could be enhanced by combining measurements ufrom the pole and at another Antarctic station such as Dome C.

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