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The structure of the lower transition region as inferred from the hydrogen Lyman-α line radiance

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

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Solanki,  S. K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
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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Curdt,  W.
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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Marsch,  E.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Teriaca, L., Schühl{}e, U., Solanki, S. K., Curdt, W., & Marsch, E. (2005). The structure of the lower transition region as inferred from the hydrogen Lyman-α line radiance. In D. E. Innes, A. Lagg, S. K. Solanki, & D. Danesy (Eds.), Proceedings of the International Scientific Conference on Chromospheric and Coronal Magnetic Fields. Noordwijk: ESA Publ. Div.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-F9E1-C
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