The observation of solar activity has problems of small field of view and low resolution. The field of view corrected by a single-conjugated adaptive optics system is small, and a multi-conjugated adaptive optics system based on the method of three-dimensional reconstruction is time-consuming and complex. However, a solar ground-layer adaptive optics system, which corrects ground-layer turbulence, can achieve high efficiency and large field of view, and obtain high-resolution images. In the case of the distribution of four star array and with the average algorithm, the YAO software is used to the numerical simulation of the solar ground-layer adaptive optical system with 40″ and 60″ optimized field of view in J and H bands, and the simulation results are compared with that of single-conjugated adaptive optics system simulation under the same conditions. The results show that Strehl ratio of the ground-layer adaptive optics system increases 130%-210% compared with that of single-conjugated adaptive optics system within imaging field of view of 60″-120″, which is consistent with the results obtained by other softwares in solar adaptive optics.