Results from previous studies indicate that the anode fall, the principal source of anode heating in MPD thrusters, increases monotonically with the electron Hall parameter calculated from electron temperature, number density, and magnetic field data obtained near the anode. In an attempt to reduce the anode fall by decreasing the local electron Hall parameter, a proof-of-concept test was performed in which an array of 36 permanent magnets were embedded within the anode of a high-power quasisteady MPD thruster to decrease the local azimuthal component of the induced magnetic field. The modified thruster was operated at power levels between 150 kW and 4 MW with argon and helium propellants. Terminal voltage, triple probe, floating probe, and magnetic probe measurements were made to characterize the performance of the thruster with the new anode. Incorporation of the modified anode resulted in a reduction of the anode fall by up to 15 V with argon and 20 V with helium, which corresponded to decreased anode power fractions of 40 and 45% with argon and helium, respectively. Nomenclature B = magnetic field strength, T e = elementary charge, 1.6 x 10~1 9 C j a = anode current density, A/cm 2 k = Boltzmann's constant, 1.38 x 1Q-23 J/K m e = electron mass, 9.11 x 10~3 1 kg n e = electron number density, m~3 q a -anode heat flux, W/cm 2 q c = anode heat flux from convection, W/cm 2 q r = anode heat flux from radiation, W/cm 2 T e = electron temperature, K V a = anode fall, V Z = axial direction £ () = permittivity of free space, 8.85 x 10~1 2 F/m 0 = azimuthal angle A = plasma parameter \ e = electron Debye length, m (| > = anode material work function, 4.62 V £l e = electron Hall parameter Introduction I T has long been established that a propulsion system of high exhaust velocity is desirable for interplanetary space missions. A review of the rocket equation shows that in order for a propulsive system not to require an inordinate amount of propellant for a given space mission, its exhaust velocity should be at least of the same order as the characteristic velocity increment required for the mission. For most interplanetary missions, a characteristic velocity increment of at least 10 km/s is necessary. 1 " 4 Because of its potential for achieving extremely large exhaust velocities (>40 km/s), the Presented as Paper 92-3461 at the AIAA/SAE/ASME/ASEE 28th