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  Observationally driven 3D MHD model of the solar corona above a magnetically active region

Bourdin, P.-A. (2013). Observationally driven 3D MHD model of the solar corona above a magnetically active region. PhD Thesis, Georg‐August‐Univ., Göttingen.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0023-D1F6-9 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0023-D1F7-7
Genre: Thesis

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 Creators:
Bourdin, Philippe-André1, 2, Author              
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              

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 Dates: 2013
 Publication Status: Published in print
 Pages: -
 Publishing info: Georg‐August‐Univ., Göttingen
 Table of Contents: -
 Rev. Method: Peer
 Identifiers: ISBN: 978‐3‐944072‐03‐6
BibTex Citekey: Bourdin:2013-044
 Degree: PhD

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