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  • Gravatar admin created the өгөгдлийн бүрдэл The Helioseismic and Magnetic Imager (HMI) vector magnetic field pipeline: Optimization of the spectral line inversion code
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Using 5bd556eb4 from branch HEAD.
Last updated 2025-02-17 13:02:01.
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Last updated 2025-06-18 16:41:00.
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This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.