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.; Leka, K. D.; Barnes, G.

doi:10.1007/s11207-014-0497-7

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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: https://hdl.handle.net/11858/00-001M-0000-0024-BA56-F Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0024-BA57-D

Genre: Journal Article

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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: Date issued: 2014

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Rev. Type: 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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Pages: - Volume / Issue: 289 Sequence Number: - Start / End Page: 3531 - 3547 Identifier: -