太阳色球层中加速质子对氦 D3 线的线性偏振作用

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
M. B. Shapochkin, S. A. Bogachev
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引用次数: 0

摘要

摘要 在这篇文章中,我们研究了在太阳耀斑中加速的质子作用下,太阳色球层中发生的氦D3线的影响线性极化。计算了质子的能量分布与在色球内移动距离的关系。从理论上确定了不同深度的非热质子和热电子的浓度比。通过计算色球层不同层氦线 D3 的线性极化程度,确定了该线可能形成的区域。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Linear Polarization of the Helium D3 Line by Accelerated Protons in the Solar Chromosphere

Linear Polarization of the Helium D3 Line by Accelerated Protons in the Solar Chromosphere

Linear Polarization of the Helium D3 Line by Accelerated Protons in the Solar Chromosphere

In the article, we have studied the impact linear polarization of the helium D3 line that takes place in the solar chromosphere under the action of protons accelerated in solar flares. The dependence of the energy distribution of protons on the distance traveled inside the chromosphere is calculated. The ratio of the concentrations of nonthermal protons and thermal electrons at different depths is theoretically determined. From the calculation of the degree of linear polarization of the helium line D3 for different layers of the chromosphere, the region of probable formation of the line is determined.

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来源期刊
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
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