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

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Mierla,  M.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Schwenn,  R.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Teriaca,  L.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Podlipnik,  B.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Mierla, M., Schwenn, R., Teriaca, L., Stenborg, G., & Podlipnik, B. (2008). Analysis of the Fe X and Fe XIV line width in the solar corona using LASCO-C1 spectral data. Astronomy and Astrophysics, 480, 509-514. doi:10.1051/0004-6361:20078329.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-FE78-0
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