The aerothermodynamic design of vehicles that will enter or reenter a
planetary atmosphere relies largely on information gathered in ground-
based simulation facilities. Owing to the different natures of the flo
w phenomena that occur along the flight path, different wind tunnels d
edicated to particular phases of the flight are usually used. Ground s
imulation of the so-called 'hot' or hypersonic phase is particularly d
ifficult because of the high powers required to generate the wind-tunn
el flow.