  HAT-P-11 is a planet-hosting K4V star in the Kepler field, with an activity
cycle that bear similarities to the Sun's. The chromospheric activity of
HAT-P-11 indicates that a new activity cycle is beginning. We report
ground-based observations with holographic diffuser photometry to measure the
starspots of HAT-P-11 in its second observed magnetic activity cycle (Cycle 1).
We find the area coverage of starspots within the transit chord for UTC
2017-10-30 is 14% --- which makes this transit the most spotted HAT-P-11
transit observed to date. We suggest that we are likely observing occultations
of large spot groups appearing at the beginning of Cycle 1.
