SphinX soft X-ray spectrophotometer: Science objectives, design and performance

被引：0

作者：

S. Gburek

J. Sylwester

M. Kowalinski

J. Bakala

Z. Kordylewski

P. Podgorski

S. Plocieniak

M. Siarkowski

B. Sylwester

W. Trzebinski

S. V. Kuzin

A. A. Pertsov

Yu. D. Kotov

F. Farnik

F. Reale

K. J. H. Phillips

机构：

[1] Polish Academy of Sciences,Space Research Center

[2] P.N. Lebedev Physical Institute of the Russian Academy of Sciences,undefined

[3] National Research Nuclear University “MEPhI”,undefined

[4] Astronomical Institute of Academy of Sciences of the Czech Republic,undefined

[5] INAF—G.S. Vaiana Astronomical Observatory,undefined

[6] Mullard Space Science Laboratory,undefined

来源：

Solar System Research | 2011年 / 45卷

关键词：

solar corona; spectrum; X-ray; abundances; instrumentation; SphinX;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

The goals and construction details of a new design Polish-led X-ray spectrophotometer are described. The instrument is aimed to observe emission from entire solar corona and is placed as a separate block within the Russian TESIS X- and EUV complex aboard the CORONAS-PHOTON solar orbiting observatory. SphinX uses silicon PIN diode detectors for high time resolution measurements of the solar spectra in the range 0.8–15 keV. Its spectral resolution allows for discerning more than hundred separate energy bands in this range. The instrument dynamic range extends two orders of magnitude below and above these representative for GOES. The relative and absolute accuracy of spectral measurements is expected to be better than few percent, as follows from extensive ground laboratory calibrations.

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