Analysis of the Fe X and Fe XIV line width in the solar corona using LASCO-C1 spectral data

M. Mierla、R. Schwenn、L. Teriaca、G. Stenborg、B. Podlipnik

2008Astronomy and AstrophysicsPhysics and Astronomy被引 33开放获取

摘要

Aims.The purpose of this paper is to analyze the variation in the line width with height in the inner corona (region above 1.1 ), by using the spectral data from LASCO-C1 aboard SOHO. We used data acquired at activity minimum (August–October 1996) and during the ascending phase of the solar cycle (March 1998).

引用本文（GB/T 7714）

M. Mierla, R. Schwenn, L. Teriaca, 等. Analysis of the Fe X and Fe XIV line width in the solar corona using LASCO-C1 spectral data[J]. Astronomy and Astrophysics, 2008.

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DOI：https://doi.org/10.1051/0004-6361:20078329

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