The Solar Optical Telescope for the Hinode Mission: An Overview

TL;DR

The Solar Optical Telescope on Hinode provides high-resolution, stable imaging of the Sun's photosphere and chromosphere, enabling advanced studies of solar magnetic phenomena with unprecedented clarity.

Contribution

This paper offers an overview of SOT's design, capabilities, and its role within the Hinode mission for solar observation.

Findings

High-resolution imaging of solar magnetic fields

Stable point spread function with error less than 0.01 arcsec

Complementary to other Hinode instruments for solar research

Abstract

The Solar Optical Telescope (SOT) aboard the Hinode satellite (formerly called Solar-B) consists of the Optical Telescope Assembly (OTA) and the Focal Plane Package (FPP). The OTA is a 50 cm diffraction-limited Gregorian telescope, and the FPP includes the narrow-band (NFI) and wide-band (BFI) filtergraphs, plus the Stokes spectro-polarimeter (SP). SOT provides unprecedented high resolution photometric and vector magnetic images of the photosphere and chromosphere with a very stable point spread function, and is equipped with an image stabilization system that reduces the error to less than 0.01 arcsec rms. Together with the other two instruments on Hinode (the X-Ray Telescope (XRT) and EUV Imaging Spectrometer (EIS)), SOT is poised to address many fundamental questions about solar magneto-hydrodynamics. Note that this is an overview, and the details of the instrument are presented in a series of companion papers.