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Recently discovered regular X-ray bursts known as quasi-periodic eruptionshave a proposed model that suggests a tidal stripping white dwarf inspirallinginto the galaxy's central black hole on an eccentric orbit. According to thismodel, the interaction of the stripping white dwarf with the central black holewould emit gravitational wave signals as well, their detection can help explorethe formation mechanism of quasi-periodic eruptions and facilitatemulti-messenger observations. In this paper, we aim to perform a preliminarystudy of the gravitation wave observation of TianQin on this stripping whitedwarf model. We investigated the horizon distance of TianQin on this type ofgravitation wave signal and found it can be set to 200Mpc. We also find thatthose stripping white dwarf model sources with central black hole mass within$10^4\sim10^{5.5}M_\odot$ are more likely to be detected by TianQin. Weassessed the parameter estimation precision of TianQin on those stripping whitedwarf model sources. Our result shows that, even in the worst case, TianQin candetermine the central black hole mass, the white dwarf mass, the central blackhole spin, and the orbital initial eccentricity with a precision of $10^{-2}$.In the optimistic case, TianQin can determine the central black hole mass andthe white dwarf mass with a precision of $10^{-7}$, determine the central blackhole spin with a precision of $10^{-5}$, and determine the orbital initialeccentricity with a precision of $10^{-8}$. Moreover, TianQin can determine theluminosity distance with a precision of $10^{-1}$ and determine the skylocalization with a precision of $10^{-2}\sim10$ $\rm deg^2$.

Observing white dwarf tidal stripping with TianQin gravitational wave observatory