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  Modeling statistical properties of solar active regions through direct numerical simulations of 3D-MHD turbulence

Malapaka, S. K., & Müller, W.-C. (2013). Modeling statistical properties of solar active regions through direct numerical simulations of 3D-MHD turbulence. The Astrophysical Journal, 774: 84 (11pp). doi:10.1088/0004-637X/774/1/84.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0026-E094-5 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0026-E095-3
Genre: Journal Article

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 Creators:
Malapaka, S. K.1, Author           
Müller, W.-C.1, Author           
Affiliations:
1External Organizations, ou_persistent22              

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Language(s): eng - English
 Dates: 2013
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Internal
 Identifiers: eDoc: 669184
DOI: 10.1088/0004-637X/774/1/84
URI: http://dx.doi.org/10.1088/0004-637X/774/1/84
URI: http://de.arxiv.org/pdf/1307.4377
 Degree: -

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Title: The Astrophysical Journal
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: The American Astrophysical Society
Pages: - Volume / Issue: 774 Sequence Number: 84 (11pp) Start / End Page: - Identifier: -