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The HMI project recently started processing the continuum intensity imagesfollowing global helioseismology procedures similar to those used to processthe velocity images. The spatial decomposition of these images has producedtime series of spherical harmonic coefficients for degrees up to $\ell=300$,using a different apodization than the one used for velocity observations. Thefirst 360 days of observations were processed and made available. In this paperI present initial results from fitting these time series using my state of theart fitting methodology and compare the derived mode characteristics to thoseestimated using co-eval velocity observations.

Initial Results from Fitting Resolved Modes using HMI Intensity Observations