Аннотация:The period near the minimum of the solar cycle 23 is characterized by the low sporadic activity and stable quasistationary high speed corotating patterns in the solar wind. The sources of high speed solar wind streams were long-living low-latitude coronal holes. The paper describes forecast of these quasi-stationary solar wind streams using different semi-empirical models based on the coronal holes characteristics as an input. The results of developed models show good correlation with the solar wind data. As well, our results were compared with widely-used Wing-Sheeley-Arge prediction model and demonstrated similar or even better performance.