The Langmuir probe has been used as an effective tool for in-situ plasma parameter measurements since the past century (Bering et al., 1973;Mott-Smith & Langmuir, 1926;. In recent decades, it has been widely carried by many Low Earth Orbit (LEO) satellites, such as the Challenging Minisatellite Payload (CHAMP) (Cooke et al., 2003), the Detection of Electromagnetic Emissions Transmitted from Earthquake Regions (DEMETER) (Lebreton et al., 2006), the Swarm satellites (Alpha, Bravo, and Charlie) (Buchert et al., 2015), and the China Seismo-Electromagnetic Satellite (CSES) (Shen et al., 2018) whose Langmuir probe data is the subject of this paper.The Langmuir probe can provide the electron density (Ne), electron temperature (Te) and plasma potential (Vp) by collecting the plasma currents (I) after applying a specific range of bias voltage (V) to the probe (Chen & Chang, 2002;Lebreton et al., 2006;Mott-Smith & Langmuir, 1926). Ne and Te are two essential parameters for describing ionosphere physics, so their reliability and accuracy directly concern scientific research. However, due to the complicated space plasma environment and the limitations of the Langmuir probe detection methods, the adverse effects of probe contamination and interferences generated onboard the satellite always need to be carefully considered (