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  The Helioseismic and Magnetic Imager (HMI) vector magnetic field pipeline: optimization of the spectral line inversion code

Centeno, R., Schou, J., Hayashi, K., Norton, A., Hoeksema, J. T., Liu, Y., et al. (2014). The Helioseismic and Magnetic Imager (HMI) vector magnetic field pipeline: optimization of the spectral line inversion code. Solar Physics, 289, 3531-3547. doi:10.1007/s11207-014-0497-7.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0024-BA56-F Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0024-BA57-D
Genre: Journal Article

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 Creators:
Centeno, R., Author
Schou, J.1, Author              
Hayashi, K., Author
Norton, A., Author
Hoeksema, J. T., Author
Liu, Y., Author
Leka, K. D., Author
Barnes, G., Author
Affiliations:
1Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              

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 MPIS_GROUPS: Solar and Stellar Interiors
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 Dates: 2014
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: DOI: 10.1007/s11207-014-0497-7
BibTex Citekey: Centeno:2014-113
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Title: Solar Physics
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 289 Sequence Number: - Start / End Page: 3531 - 3547 Identifier: -