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Why are coronal holes indistinguishable from the quiet sun in transition region radiation?

MPS-Authors
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Wiegelmann,  T.
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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Wiegelmann, T., & Solanki, S. K. (2004). Why are coronal holes indistinguishable from the quiet sun in transition region radiation? In R. W. Walsh, J. Ireland, D. Danesy, & B. Fleck (Eds.), Proc. SOHO 15 `Coronal Heating' (pp. 35-40). Noordwijk: ESA Publ. Div.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-F173-2
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