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  A quantitative method to optimise magnetic field line fitting of observed coronal loops

Carcedo, L., Brown, D. S., Hood, A. W., Neukirch, T., & Wiegelmann, T. (2003). A quantitative method to optimise magnetic field line fitting of observed coronal loops. Solar Physics, 218, 29-40.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-EF03-2 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-EF04-F
Genre: Journal Article

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Carcedo, L., Author
Brown, D. S., Author
Hood, A. W., Author
Neukirch, T., Author
Wiegelmann, T.1, Author           
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              

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 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: STEREO: SECCHI
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 Dates: 2003
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: BibTex Citekey: Carcedo:2003-163
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Title: Solar Physics
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 218 Sequence Number: - Start / End Page: 29 - 40 Identifier: -