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The Sun provides the energy necessary to sustain our existence. While the Sunprovides for us, it is also capable of taking away. The weather and climaticscales of solar evolution and the Sun-Earth connection are not well understood.There has been tremendous progress in the century since the discovery of solarmagnetism - magnetism that ultimately drives the electromagnetic, particulateand eruptive forcing of our planetary system. There is contemporary evidence ofa decrease in solar magnetism, perhaps even indicators of a significantdownward trend, over recent decades. Are we entering a minimum in solaractivity that is deeper and longer than a typical solar minimum, a "grandminimum"? How could we tell if we are? What is a grand minimum and how does theSun recover? These are very pertinent questions for modern civilization. Inthis paper we present a hypothetical demonstration of entry and exit from grandminimum conditions based on a recent analysis of solar features over the past20 years and their possible connection to the origins of the 11(-ish) yearsolar activity cycle.

Deciphering Solar Magnetic Activity: On Grand Minima in Solar Activity