The day/night cycle at a single observatory prevents definitive observ
ations of many aspects of solar activity, convection, and oscillations
with timescales near 1 day. Solutions to this problem include multi-s
ite networks, spacecraft observatories, and observations from high-lat
itude sites during their summer season. We report here on our experien
ce in using Alaska as a high-latitude site for observations of solar o
scillations.