Voyager data led to a new theory that the heliosheath has "magnetic bubbles" and a stagnation zone.

In mathematics, when the fluid flows through thin and long tubes it forms stagnation zones where the flow becomes almost immobile.

Below the splitter, the air is redirected away from the stagnation zone and is accelerated, causing the pressure to drop.

Voyager 1 has confirmed the existence of a "stagnation zone" where the influences of the Sun and interstellar space largely balance out.

Apriori information regarding the stagnation zones contributes to optimization of the computational process by replacing the unknown functions with the corresponding constants in such zones.

Identification of what parameters impact the sizes of stagnation zones opens up opportunities for practical recommendations on targeted changes in configuration (reduction or increase) of such zones.

If the coast is rugged with headlands, a mosaic of complex flow fields consisting of eddies, jets, and stagnation zones will occur, further complicating the circulation patterns outside of the estuary.

Studies have shown that in the Sea of Azov, the exact vertical structure is dependent on wind strength and sea surface temperature, but typically a 'stagnation zone' lies between the oxic and anoxic layers.

Stagnation zones theorems are closely related to pre-Liouville's theorems about evaluation of solutions fluctuation, which direct consequences are the different versions of the classic Liouville theorem about conversion of the entire doubly periodic function into the identical constant.

For example, if the subarc of a domain boundary has zero transparency, and the flow of the gradient vector field of the function through the rest of the boundary is small enough, then the domain for such function is its stagnation zone.