What is Heliopause?
The heliopause is the theoretical border where the Sun's solar wind is stopped by the interstellar medium. It defines the outer boundary of the heliosphere, the vast magnetic bubble surrounding our solar system. At this boundary, the outward dynamic pressure of the ionized gas (plasma) ejected by the Sun balances the inward pressure of the interstellar gas and magnetic fields from the Milky Way galaxy: P solar wind = P interstellar medium Structure of the Heliospheric Boundary The transition from solar dominance to interstellar space occurs across three primary layers: Termination Shock: The inner boundary where the supersonic solar wind abruptly slows down to subsonic speeds as it collides with the interstellar medium, causing intense turbulence and heating. Heliosheath: The thick, highly turbulent region beyond the termination shock where the slowed solar wind interacts directly with incoming interstellar gas. Heliopause: The sharp outer surface of the heliosheath wher...