The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance

The Helioseismic and Magnetic Imager (HMI) began near-continuous full-disk solar measurements on 1 May 2010 from the Solar Dynamics Observatory (SDO). An automated processing pipeline keeps pace with observations to produce observable quantities, including the photospheric vector magnetic field, fro...

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Veröffentlicht in:	Solar physics 2014-09, Vol.289 (9), p.3483-3530
Hauptverfasser:	Hoeksema, J. Todd, Liu, Yang, Hayashi, Keiji, Sun, Xudong, Schou, Jesper, Couvidat, Sebastien, Norton, Aimee, Bobra, Monica, Centeno, Rebecca, Leka, K. D., Barnes, Graham, Turmon, Michael
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics and Astroparticles Atmospheric Sciences Disks Fields (mathematics) Filtergrams Inversions Magnetic fields Mathematical analysis Noise reduction Physics Physics and Astronomy Pipelines Solar activity Solar Cycle 24 as seen by SDO Solar physics Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Vectors (mathematics) Wavelengths
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