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

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Schou, J.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0024-BA56-F

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