The Dungey cycle, officially proposed by James Dungey in 1961,[1] is a phenomenon that explains interactions between a planet's magnetosphere and solar wind.[2] Dungey originally proposed a cyclic behavior of magnetic reconnection between Earth's magnetosphere and flux of solar wind. This reconnection explained previously observed dynamics within Earth's magnetosphere.[3] The rate of reconnection in the beginning of the cycle is dependent on the orientation of the interplanetary magnetic field[4] as well as the resultant plasma conditions at the site of reconnection. On Earth, the reconnection cycle takes around 1 hour, but this differs from planet to planet.