Wavelength Determination for Solar Features Observed by the EUV Imaging Spectrometer on Hinode
Wavelength Determination for Solar Features Observed by the EUV Imaging Spectrometer on Hinode
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Hinode 上的 EUV 成像光谱仪观测到的太阳特征的波长测定
DOI：
10.1093/pasj/59.sp3.s865
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发表时间：
2007
影响因子：
2.3
通讯作者：
J. Davila
中科院分区：
文献类型：
--
作者：
C. Brown;H. Hara;S. Kamio;U. Feldman;J. Seely;G. Doschek;J. Mariska;C. Korendyke;J. Lang;K. Dere;L. Culhane;R. Thomas;J. Davila
报道了日之出卫星上高分辨率极紫外成像光谱仪（EIS）观测到的太阳谱线的波长定标。对宁静太阳和两个轻度活动区域的光谱特征进行了测量和校准。列出了观察到的更强谱线以及主要贡献离子的鉴别。报告了41条线，其中90%被识别。波长精度（2 σ）为± 0.0031埃（EIS短波段）和± 0.0029埃（EIS长波段）。这些谱线是1- 2x 10 {sup 6} K等离子体的典型谱线，建议作为建立EIS波长标度的标准。EIS的温度在轨道周围变化约1.5摄氏度，也与航天器指向有关。这些温度变化与波长与像素数尺度变化的相关性报告。
A wavelength calibration of solar lines observed by the high resolution EUV Imaging Spectrometer (EIS) on the Hinode satellite is reported. Spectral features of the quiet sun and of two mildly active areas were measured and calibrated. A listing of the stronger observed lines with identification of the leading contributor ions is presented. 41 lines are reported, with 90% identified. Wavelength precisions (2{sigma}) of {+-}0.0031 Angstroms for the EIS short band and {+-}0.0029 Angstroms for the EIS long band are obtained. These lines, typical of 1-2x10{sup 6} K plasmas, are recommended as standards for the establishment of EIS wavelength scales. The temperature of EIS varies by about 1.5 C around the orbit and also with spacecraft pointing. The correlation of these temperature changes with wavelength versus pixel number scale changes is reported.
影响因子：
2.8
作者：
Kosugi, T.;Matsuzaki, K.;Golub, L.
通讯作者：
Golub, L.