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  Evolution of relative magnetic helicity: method of computation and application to a simulated solar corona above an Active Region

Yang, S., Büchner, J., Sanos, J. C., & Zhang, H. (2013). Evolution of relative magnetic helicity: method of computation and application to a simulated solar corona above an Active Region. Solar Physics, 283, 369-382. doi:10.1007/s11207-013-0236-5.

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 Creators:
Yang, Shangbin1, Author           
Büchner, Jörg1, 2, Author           
Sanos, Jean Carlo, Author
Zhang, Hongqi, 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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 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: Theory: Sim Sol Sys Plasma
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 Dates: 2013
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: DOI: 10.1007/s11207-013-0236-5
BibTex Citekey: Yang:2013-022
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Title: Solar Physics
Source Genre: Journal
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Pages: - Volume / Issue: 283 Sequence Number: - Start / End Page: 369 - 382 Identifier: -