  We present an overview of K2 short cadence observations for 34 M dwarfs
observed in Campaigns 1 - 9 which have spectral types between M0 - L1. All of
the stars in our sample showed flares with the most energetic reaching
$3\times10^{34}$ ergs. As previous studies have found, we find rapidly rotating
stars tend to show more flares, with evidence for a decline in activity in
stars with rotation periods longer than approximately 10 days. We determined
the rotational phase of each flare and performed a simple statistical test on
our sample to determine whether the phase distribution of the flares is random
or if there is a preference for phase. We find, with the exception of one star
which is in a known binary system, that none show a preference for the
rotational phase of the flares. This is unexpected and all stars in our sample
show flares at all rotational phases, suggesting these flares are not all
originating from one dominant starspot on the surface of the stars. We outline
three scenarios which could explain the lack of a correlation between the
number of flares and the stellar rotation phase. In addition we also highlight
preliminary observations of DP Cnc, observed in campaigns 16 and 18, and is one
of the stars in our extended sample from K2 Campaigns 10 -18 which are still to
be examined.
