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The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)medium-resolution spectral survey of Galactic Nebulae (MRS-N) has conducted forthree years since Sep. 2018 and observed more than 190 thousands nebularspectra and 20 thousands stellar spectra. However, there is not yet a dataprocessing pipeline for nebular data. To significantly improve the accuracy ofnebulae classification and their physical parameters, we developed the MRS-NPipeline. This article presented in detail each data processing step of theMRS-N Pipeline, such as removing cosmic rays, merging single exposure, fittingsky light emission lines, subtracting skylight, wavelength recalibration,measuring nebular parameters, creating catalogs and packing spectra. Finally, adescription of the data products, including nebular spectra files and parametercatalogs, is provided.

The Data Processing of the LAMOST Medium-Resolution Spectral Survey of Galactic Nebulae (LAMOST MRS-N Pipeline)