Release Notes for Initial Milne Eddington Inversion of HMI Magnetic Field Data (VFISV)

hmi.ME_720s_e15w1332 ([http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.ME_720s_e15w1332 click here for data]) and hmi.ME_720s_e15w1332_HARP ([http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.ME_720s_e15w1332_HARP click here for data])

These two data series contain ME inversion data processed using VFISV ([http://hmi.stanford.edu/doc/magnetic/section4.pdf details]) using the codes implemented through 27 November, 2011. There are known issues with these versions of VFISV, but this remains the best ME release version as of February 27, 2012.

Our efforts to optimize the VFISV for the HMI data pipeline are on going, and we will create the series to fill the data processed by the newer codes when ready. We will announce the release of the new data through Solar News.

Temporal ''coverage charts'' for these two series

Charts in [http://jsoc.stanford.edu/doc/data/hmi/coverage_maps/inversion/ this directory] show the 12-minute time slots for which the ME inversion data processed with the VFISV module are available. The coverage charts also contain the status flags of the HMI observation, thus the quality and availability of input [http://jsoc.stanford.edu/ajax/lookdata.html?ds=hmi.S_720s Stokes] data. See [:ME720se15w1332CoverChart: details] for an explanation of the coverage charts.

Versions of VFISV in the FITS files exported at JSOC database