The solar optical telescope of Solar-B (Hinode): The optical telescope assembly
The Solar Optical Telescope (SOT) aboard the Solar-B satellite (Hinode) is designed to perform high-precision photometric and polarimetric observations of the Sun in visible light spectra (388-668 nm) with a spatial resolution of 0.2-0.3 arcsec. The SOT consists of two optically separable components: the Optical Telescope Assembly (OTA), consisting of a 50-cm aperture Gregorian with a collimating lens unit and an active tip-tilt mirror, and an accompanying Focal Plane Package (FPP), housing two filtergraphs and a spectro-polarimeter. The optomechanical and optothermal performance of the OTA is crucial to attain unprecedented high-quality solar observations. We describe in detail the instrument design and expected stable diffraction-limited on-orbit performance of the OTA, the largest state-of-the-art solar telescope yet flown in space.
document
https://n2t.org/ark:/85065/d7hq403w
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2008-06-01T00:00:00Z
An edited version of this paper was published by Springer. Copyright 2008, Springer Netherlands
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