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

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.

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 Creators:
Wiegelmann, T.1, Author              
Solanki, S. K.1, 2, Author              
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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Free keywords: -
 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: Theory: MHD Solar
 Abstract: -

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 Dates: 2004
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: BibTex Citekey: Wiegelmann:2004-236
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Title: Proc. SOHO 15 `Coronal Heating'
Source Genre: Proceedings
 Creator(s):
Walsh, R. W., Editor
Ireland, J., Editor
Danesy, D., Editor
Fleck, B., Editor
Affiliations:
-
Publ. Info: Noordwijk : ESA Publ. Div.
Pages: - Volume / Issue: (ESA SP-575) Sequence Number: - Start / End Page: 35 - 40 Identifier: -