On the fine structure of the Fe I λ532.4185-nm line profile in the spectrum of the solar disk center

被引：0
|
作者：
D. M. Kuli-Zade
Z. F. Shabanova
机构：
[1] Baku State University,
来源：
Kinematics and Physics of Celestial Bodies | 2008年 / 24卷 / 6期
关键词：
Solar Phys; Line Profile; Celestial Body; Equivalent Width; Convective Motion;
D O I：
10.3103/S0884591308060056
中图分类号：
学科分类号：
摘要：
Based on the digital spectra taken with double monochromators of high spectral resolution, we have constructed the profile of the Fe I λ532.4185-nm line in the spectrum of the solar disk center. Basic spectrophotometric characteristics of the line profile have been determined with a high accuracy. The fine structure of the line profile is studied in detail. The profile asymmetry parameters have been determined.
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页码：296 / 299
页数：3
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