  We exploit more than 1000 star cluster Monte Carlo models from the
MOCCA-SURVEY Database I, to infer the local rate density of white dwarf (WD)
tidal disruption events (TDEs) in globular clusters (GCs) and young massive
clusters (YMCs). We suggest that the WD TDE rate for GCs and YMCs in the local
universe is $\sim 90$-$500~{\rm yr}^{-1}~{\rm Gpc}^{-3}$, with 90 % of WD TDEs
occurring in GCs. The total WD TDE rate density is $\sim 9$-$50$ times larger
than estimated before. Our results show that thermonuclear explosions induced
by WD TDEs can be observed at a rate of $\sim 100$-$550~{\rm yr}^{-1}$ by the
next generation optical surveys, such as the Legacy Survey of Space & Time by
the Vera C. Rubin Observatory. We also find that massive WDs are preferentially
disrupted due to mass segregation, and that 20 % of exploding WDs have $\gtrsim
1.0 M_\odot$ despite of the small population of such WDs.
