This paper continues a larger study concerning the cyclic behaviour of the High Speed Plasma Streams (HSPSs). All the streams were classified as co-rotating streams and flare-generated streams, using the characteristics of the streams. For the solar cycle (SC) 22 (1986 ― 1996) the following parameters of HSPSs were yearly calculated: the sum of durations (in days); the sum of maximum velocities; the sum of the velocity gradients; the sum of the importances of the streams. Geomagnetic variations during the period 1986 ― 1996 are analyzed, too. All the HSPSs present the greatest values of the all parameters during the second part of the descending branch of the SC 22. There also are some secondary maxima of the HSPS intensity before and after the maximum of the solar cycles, 1987 and 1991, respectively. The maxima are discussed related to the HSPSs' origin and in correlation with the geomagnetic variations.
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