Assertion: heliosphere's wind | /r/CapableOf | slow down to subsonic speed
Facets:
Source sentences:
text: The termination shock is the point in the heliosphere where the solar wind slows down to subsonic speed (relative to the Sun) because of interactions with the local interstellar medium.
text: The first feature encountered by a spacecraft as a result of this interstellar wind–solar wind interaction was the termination shock where the solar wind slows to subsonic speed and large changes in plasma flow direction and magnetic field orientation occur.
text: Nearer the Sun than the heliopause lies the heliosheath, a region of transition where the solar wind slows to subsonic speeds—that is, slower than the speed with which disturbances travel through the interstellar medium.
text: The termination shock is the point in the heliosphere where the solar wind slows down to subsonic speed.
text: In 2004 Voyager passed the termination shock – the point in the heliosphere where the solar wind slows down to subsonic speed (relative to other stars) because of interactions with the local interstellar medium.
text: The first feature encountered by a spacecraft as a result of this interstellar wind–solar wind interaction was the termination shock where the solar wind slows to subsonic speed and large changes in plasma flow direction and magnetic field orientation occur.
text: This marks the point where the solar wind slows to subsonic speeds.