  DW Cnc is an intermediate polar which has previously been observed in both
high and low states. Observations of the high state of DW Cnc have previously
revealed a spin period at ~ 38.6 min, however observations from the 2018/19 low
state showed no evidence of the spin period. We present results from our
analysis of 12 s cadence photometric data collected by NGTS of DW Cnc during
the high state which began in 2019. Following the previously reported
suppression of the spin period signal we identify the return of this signal
during the high state, consistent with previous observations of it. We identify
this as the restarting of accretion during the high state. We further
identified three short outbursts lasting ~ 1 d in DW Cnc with a mean recurrence
time of ~ 60 d and an amplitude of ~ 1 mag. These are the first outbursts
identified in DW Cnc since 2008. Due to the short nature of these events we
identify them not as a result of accretion instabilities but instead either
from instabilities originating from the interaction of the magnetorotational
instability in the accretion disc and the magnetic field generated by the white
dwarf or the result of magnetic gating.
