The sun’s solar wind is a flowing continuum of plasma that rarely enmeshes with the forces of the Earth’s magnetic field. But when one’s protons and electrons collide with the particles in the other’s airspace, the night sky appears galvanised with a string of electric projections, parading spectrums of magenta, sapphire, and cerulean. Whereby such celestial events cause a stir amongst those hoping to ogle at the Aurora Borealis – more commonly termed “The Northern Lights” – the conditions for its visibility rely partly on the onlooker’s northernmost positioning, but foremost, a twist of fate.