During the deep space exploration of the solar system, the reliable communication link is vital, since it is the only way that enables the transmission of telecommand from the earth and the return of telemetry information and scientific data from the probe. However, the communication link in the solar system space environment faces many severe challenges. In addition, due to the ultralong communication distance, the communication link between the Earth and the solar system probe may encounter solar scintillation due to solar wind during near superior solar conjunction (Morabito & Hastrup, 2001). Solar scintillation is a telecommand and telemetry signal fluctuation phenomenon. When the transmitted telecommand and telemetry signals pass through the solar corona region, the solar wind causes telecommand and telemetry signal amplitude fluctuation, phase fluctuation and spectrum expansion. Especially, if the solar scintillation is sufficiently strong that means the heliocentric distance is less than four solar radii(Xu & Song, 2019), the communication link may be intermittently or even completely interrupted, which results in communication failure