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The dynamic nature of the solar transition region as revealed by spectroscopy of the hydrogen Lyman-alpha line

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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Schühle,  U.
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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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., Schühle, U., Solanki, S. K., Curdt, W., & Marsch, E. (2006). The dynamic nature of the solar transition region as revealed by spectroscopy of the hydrogen Lyman-alpha line. In H. Lacoste (Ed.), Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy. Noordwijk: ESA Publ. Div.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-FADB-3
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