Magnetars are the most powerful compact objects in the stellar mass
range observed in the Milky Way.  Magnetars are young neutron stars with
high surface magnetic fields, exceeding around 10 TeraGauss. They
exhibit persistent soft X-ray signals that emanate from their surfaces,
and striking, powerful flares that must originate in their
magnetospheres.  This year, a Galactic magnetar SGR J1935+2154 became
very active and emitted a bright, fast radio burst (FRB).  This is the
first source association for FRBs, which are almost exclusively of
distant extragalactic origin.  Intriguingly, the FRB was contemporaneous
with an unusual X-ray burst.  This talk summarizes the X-ray burst
landscape for the burst storm from this magnetar, providing context for
interpreting the magnetospheric locale of the FRB