Post-focus instrumentation for GREGOR

Details Post-focus instrumentation for GREGOR Post-focus instrumentation for GREGOR

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001an....322..361k&link_type=abstract

Astronomische Nachrichten, vol. 322, no. 5/6, p. 361-362

Physics

Optics

1

Scientific paper

GREGOR is a high-resolution solar telescope with an aperture of 1.5 m. It will be equipped with an Adaptive Optics system and is designed for high-precision measurements of magnetic fields and plasma motions in the solar photosphere and chromosphere with a resolution of 70 km on the Sun. GREGOR will replace the Gregory Coudé Telescope at the Observatorio del Teide on Tenerife. In concert with the other solar telescopes at Teide Observatory it will be useful for studying the dynamics of the solar atmosphere and the underlying physical processes. GREGOR will also serve as a test bed for next generation solar telescopes. We discuss briefly the postfocus instrumentation of GREGOR.

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