THE SOFT-X-RAY TELESCOPE FOR THE SOLAR-A MISSION

被引：1055

作者：

TSUNETA, S

ACTON, L

BRUNER, M

LEMEN, J

BROWN, W

CARAVALHO, R

CATURA, R

FREELAND, S

JURCEVICH, B

MORRISON, M

OGAWARA, Y

HIRAYAMA, T

OWENS, J

机构：

[1] LOCKHEED PALO ALTO RES LABS,PALO ALTO,CA 94304

[2] INST SPACE & ASTRON SCI,SAGAMIHARA,JAPAN

[3] NATL ASTRON OBSERV JAPAN,MITAKA,TOKYO 181,JAPAN

[4] NASA,GEORGE C MARSHALL SPACE FLIGHT CTR,HUNTSVILLE,AL 35812

来源：

SOLAR PHYSICS | 1991年 / 136卷 / 01期

关键词：

D O I：

10.1007/BF00151694

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Soft X-ray Telescope (SXT) of the SOLAR-A mission is designed to produce X-ray movies of flares with excellent angular and time resolution as well as full-disk X-ray images for general studies. A selection of thin metal filters provide a measure of temperature discrimination and aid in obtaining the wide dynamic range required for solar observing. The co-aligned SXT aspect telescope will yield optical images for aspect reference, white-light flare and sunspot studies, and, possibly, helioseismology. This paper describes the capabilities and characteristics of the SXT for scientific observing.

引用

页码：37 / 67

页数：31

共 23 条

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