«On suborbital time scales,
ice distributions varied in the Holo - cene, but no evidence exists for large, pan-Arctic fluctuations.
Not exact matches
The
distribution of the flow types
varies with latitude — and the researchers think this means different surface layers of the asteroid contain different amounts of
ice.
We know LOD
varies continually, partly a function of seasonal
distribution of
ice mass and partly a function of variable magnetic coupling betwixt sun and earth.