Wavelengths and intensities of spectral lines in the 171-211 and 245-291 Å ranges from five solar regions recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode

被引：138

作者：

Brown, C. M. ^{[1
]}

Feldman, U. ^{[1
,3
]}

Seely, J. F. ^{[1
]}

Korendyke, C. M. ^{[1
]}

Hara, H. ^{[2
]}

机构：

[1] USN, Res Lab, Washington, DC 20375 USA

[2] Natl Astron Observ, Mitaka, Tokyo 181, Japan

[3] Artep Inc, Ellicott City, MD 21042 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2008年 / 176卷 / 02期

基金：

英国科学技术设施理事会;

关键词：

instrumentation : spectrographs; line : identification; Sun : corona; Sun : UV radiation;

D O I：

10.1086/529378

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present spectral line wavelengths, identifications, and intensities in the 171-211 and 245-291 angstrom ranges from five solar plasma regions recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode. The recorded data were emitted from a quiet region, two active areas on the solar disk, a limb region, and a region 2000 above the limb. The line list contains 500 lines of which 55% were identified with previously known transitions. Although the EIS spectral coverage is limited to two ranges approximately 40 angstrom wide, the identified lines belong to a total of 56 ions from 15 elements.

引用

页码：511 / 535

页数：25

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