The sun has a heartbeat. Every 10 or 12 years it beats, and it beats hard. This is known as the solar cycle and is measured by the number of sunspots visible on the sun. The more sunspots, the more solar flare energy is being released into space which means more aurora activity!
A: We are on the backside of Solar Cycle 24. The sunspot count is declining but 2017 still holds great potential (I have two words for you: coronal hole). I remember from Solar Cycle 23, which peaked in 2001, that some very awe-inspiring displays occurred on the downswing...which is where we are now. Never lose hope! There is aurora activity throughout the cycle. You just might have to stay up later or stay out longer to catch it which makes it that much more rewarding.
A: Between 11pm and 2am are the peak aurora hours but they can show up anytime from dusk until dawn. Some of the most colorful displays I've ever seen occurred in dawn's early twilight around 5am-7am.
Statistically, the equinox months of September and March are the best for aurora activity but the winter months of October-thru-February are also good. In northern latitudes like Fairbanks, Alaska the summer months of May, June & July are too bright to see the aurora. It's challenging to pinpoint the exact timing of a big display. The best advice I can give is to be patient, diligent and pay close attention to the websites that monitor space weather then go for it when the timing seems right. Luck favors the prepared.
SIDC-team, World Data Center for the Sunspot Index, Royal Observatory of Belgium,
Monthly Report on the International Sunspot Number,
online catalogue of the sunspot index: http://www.sidc.be/sunspot-data/, ‘1750-2017’