Comet Levy 1990c was observed from 16 to 25 August 1990 at the Observatory Hoher List, Daun, Germany, using a focal reducer and a CCD camera, giving a field of view of ∼25 arcmin. The heliocentric distance of the comet was 1.46 AU; its geocentric distance was 0.47 AU. A Fabry-Perot etalon with a fixed gap of 0.9 mm was used in imaging mode to measure the Doppler shift of the emission lines of the cometary H 2O + ions at 6159 Å, allowing the determination of the line-of-sight velocity of ions in the plasma tail. Two-dimensional fields of the ion Doppler speed in the plasma tail out to 10 6 km from the nucleus have been derived for 4 nights. To compare the velocity fields with the optical appearance of the cometary plasma tail, images taken through a narrow-band interference filter at 6159 Å were also obtained, alternating with velocity measurements. The change of the appearance from one image to another has been computed using measured velocities and compared with the observed appearance. Structures were transported to the position where they were actually observed in the following image, showing that they move by real particle motions and are not caused by wave compressions. A mean H 2O + production rate of 1.5 × 10 27 sec -1 has been derived. The comparison of the derived production rate to the value expected from photoionization rates shows that only a small portion of the ions is concentrated in the inner plasma tail and visible in our groundbased observations, in agreement with results obtained by the ICE spacecraft.