The Solar Optical Telescope of Solar-B (Hinode):: The optical telescope assembly

被引：362

作者：

Suematsu, Y. ^{[1
]}

Tsuneta, S. ^{[1
]}

Ichimoto, K. ^{[1
]}

Shimizu, T. ^{[1
,2
]}

Otsubo, M. ^{[1
]}

Katsukawa, Y. ^{[1
]}

Nakagiri, M. ^{[1
]}

Noguchi, M. ^{[1
]}

Tamura, T. ^{[1
]}

Kato, Y. ^{[1
]}

Hara, H. ^{[1
]}

Kubo, M. ^{[2
]}

Mikami, I. ^{[3
]}

Saito, H. ^{[3
]}

Matsushita, T. ^{[3
]}

Kawaguchi, N. ^{[3
]}

Nakaoji, T. ^{[3
]}

Nagae, K. ^{[3
]}

Shimada, S. ^{[4
]}

Takeyama, N. ^{[5
]}

Yamamuro, T. ^{[5
]}

机构：

[1] Natl Astron Observ Japan, Tokyo 1818588, Japan

[2] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan

[3] MELCO, Commun Syst Ctr, Amagasaki, Hyogo 6618661, Japan

[4] MELCO, Kamakura Works, Kanagawa 2478520, Japan

[5] Genesia Crop, Tokyo 1810013, Japan

来源：

SOLAR PHYSICS | 2008年 / 249卷 / 02期

基金：

英国科学技术设施理事会;

关键词：

Sun : instrumentation; Sun : space telescope; Sun : visible light;

D O I：

10.1007/s11207-008-9129-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：197 / 220

页数：24

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