The X-ray telescope (XRT) for the Hinode mission

被引：629

作者：

Golub, L.

DeLuca, E.

Austin, G.

Bookbinder, J.

Caldwell, D.

Cheimets, P.

Cirtain, J.

Cosmo, M.

Reid, P.

Sette, A.

Weber, M.

Sakao, T.

Kano, R.

Shibasaki, K.

Hara, H.

Tsuneta, S.

Kumagai, K.

Tamura, T.

Shimojo, M.

McCracken, J.

Carpenter, J.

Haight, H.

Siler, R.

Wright, E.

Tucker, J.

Rutledge, H.

Barbera, M.

Peres, G.

Varisco, S.

机构：

[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

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

[3] Natl Astron Observ, Tokyo 1818588, Japan

[4] Natl Astron Observ, Nobeyama Solar Radio Observ, Minamisa Ku, Nagano 3841305, Japan

[5] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA

[6] Osservatorio Astron Palermo GS Vaiana, I-90134 Palermo, Italy

来源：

SOLAR PHYSICS | 2007年 / 243卷 / 01期

基金：

英国科学技术设施理事会;

关键词：

D O I：

10.1007/s11207-007-0182-1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft's onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper.

引用

页码：63 / 86

页数：24

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